Function dustem_plugin_stellar_population, key=key, val=val, scope=scope, paramtag=paramtag,help=help 

;+
; NAME:

;    dustem_plugin_stellar_population

; PURPOSE:
;    Produces a system variable called '!dustem_composite_stellar_population' in which a structure containing parameters pertaining to (a) stellar population(s) is placed
; CATEGORY:
;    DUSTEM Wrapper
; CALLING SEQUENCE:

;    dustem_create_plugin_population(key=key,val=val)

; INPUTS:
;    None
; OPTIONAL INPUT PARAMETERS:
;    key  = input parameter number
;    val  = input parameter value
; OUTPUTS:
;    None
; OPTIONAL OUTPUT PARAMETERS:
;    None
; ACCEPTED KEY-WORDS:
;    help                  = if set, print this help
; COMMON BLOCKS:
;    None
; SIDE EFFECTS:
;    None
; RESTRICTIONS:
;    The dustem fortran code must be installed
;    The dustem idl wrapper must be installed
; PROCEDURE:
;    This is a dustem plugin
;-

;- HISTORY: ADDED STELLAR LUMINOSITY CLASSES

IF keyword_set(help) THEN BEGIN

  doc_library,'dustem_plugin_stellar_population'

  goto,the_end
ENDIF

scope='STELLAR_POPULATION'

paramtag=['R_star (R_sol)','T_BB (K)','D (pc)','N_stars']

;DATA IS NOW RETRIEVED FROM THIS TEXT FILE: "A Modern Mean Dwarf Stellar Color and Effective Temperature Sequence"  
;NB: intermediate spectral classes '.5' are not taken into account - this will probably have to change
;NB: Also contact the one who wrote the text file because he said so in it.
 
file = '/Users/ilyeschoubani/DUSTEM_WRAP/src/idl/EEM_dwarf_UBVIJHK_colors_Teff.txt'
frmt = '(A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A,A)'

readcol, file, V1,V2,V3,V4,V5,V6,V7,V8,V9,V10,V11,V12,V13,V14,V15,V16,V17,V18,V20,V21,V22,V23,V24,V25,V26,V27,V28,V29,V30,V31,V32, format=frmt, delim=' ', comment='#',/nan

;Paramters that are needed for the BB approximation (horrible approximation even for MS stars)
SpecType_MS = V1
T_eff_MS = V2
R_star_MS = V7

;Other parameters of other luminosity classed are being looked into. 
;BB approximation is a first degree 'bad' approximation because of the lack of radiative transfer especially at the 
;photosphere of stars. 

;REMARKS: BECAUSE I STILL HAVEN'T SET THE DEFAULT VALUE FOR THE MAJORIY OF THE STELLAR POULATIONS, I WILL COMMENT THE CORRESPONDING LINES INSTEAD OF CHOOSING ARBITRARY VALUES. 

;CONSIDERED STARS: SPEC_TYPE(4) = OBAFG, LUM_CLASS(10) = IA+,IA,IAB,IB,II,III,IV,V,VI,VII 

;===========Initializing the defaut stellar population structure===========

one_pop={radius:0.,temperature:0.,distance:0.,nstars:0.,popid:''} 

;===========Counters===========
popnumber = 0.
counto = 0.
countb = 0.
counta = 0.
countf = 0.
countg = 0.
;==============================

;REPLACE THIS WHITH A PLUGIN PARAMETER THAT CAN BE FITTED 

;===========Specifying whether to add the Mathis field (and its scaling via G0) to the composite ISRF===================
ismathis=0 ;this value will have to be manually changed at the present moment
defsysv, '!ismathis', ismathis
;====================================================================================================================== 

;===========Constants (in cgs)========== (except for the stellar population distance (in pc))
rsun2cm = 6.957e10 

;Stelar density constant to automate the computation of the number of stars. (It links the distance and the number of stars)
;The below stellar density will have to be modified as the density goes up towards the center, in globular clusters and goes down as we move out of the galactic plane
stellar_density = 0.14 ;stars/pc^3 stellar density in the SOLAR VICINITY     
;============================================================================================ 
 
;================NOTA BENE========================================================================== 
;KM are not included because I assumed that their UV part was not that important to excite the dust. 
;This will help ease and shorten the fitting procedure

;NOW THAT WE HAVE THE DATA SHOULD WE INCLUDE THEM? 

;===================================================================================================

IF keyword_set(key) THEN BEGIN 
    

    lumclass = (strmid(key,2)).remove(-1) ; extracting the luminosity class strings 
    params = strmid(key,0,/reverse_offset) ; extracting the indices (in the 'key' array) of the stellar parameters to fit  

    ; Locating the O3 stellar population parameters - this new code structure accounts for the presence of different luminosity classes.

    testo3 = strupcase(strmid(key,0,2)) EQ 'O3' ;NB: test is like this so that user can use lowercase for spectral class

    ind = where(testo3,countindo3) 

    
    ; retrieveing the defaut values from the txt database
    tsto3 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O3' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto3,ctdato3)
    if ctdato3 ne 0 then begin
        
        T_eff_MS_o3 = double(T_eff_MS(indat))
        R_star_MS_o3 = double(R_star_MS(indat))
        
    endif
    

    IF countindo3 NE 0 THEN BEGIN 

        lumclasso3 = lumclass(ind)
        nlmo3 = n_elements(lumclasso3)
        indo3_1 = fltarr(nlmo3)
        indo3_2 = indo3_1
        indo3_3 = indo3_1
        indo3_4 = indo3_1  
        countindo3_1 = indo3_1
        countindo3_2 = indo3_1 
        countindo3_3 = indo3_1
        countindo3_4 = indo3_1  
        FOR i=0L,nlmo3-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo3_1[i] =  where(testo3 and params EQ 1, countindo3_1x); index of radius of this stellar population in the val array
            countindo3_1[i] = countindo3_1x
            indo3_2[i] =  where(testo3 and params EQ 2, countindo3_2x); index of temperature of this stellar population in the val array
            countindo3_2[i] = countindo3_2x
            indo3_3[i] =  where(testo3 and params EQ 3, countindo3_3x); index of distance of this stellar population in the val array
            countindo3_3[i] = countindo3_3x
            indo3_4[i] =  where(testo3 and params EQ 4, countindo3_4x); index of the nstars of this stellar population in the val array (Q: does it make sense to have an nstars>1.? If not upper limiting it in the general fitting procedure might be handy)
            countindo3_4[i] = countindo3_4x
        ENDFOR  

    ENDIF
    
    ; Locating the O4 stellar population parameters

    testo4 = strupcase(strmid(key,0,2)) EQ 'O4'

    ind = where(testo4,countindo4)

    
    ; retrieveing the defaut values from the txt database
    tsto4 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O4' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto4,ctdato4)
    if ctdato4 ne 0 then begin
        
        T_eff_MS_o4 = double(T_eff_MS(indat))
        R_star_MS_o4 = double(R_star_MS(indat))
        
    endif

    IF countindo4 NE 0 THEN BEGIN 

        lumclasso4 = lumclass(ind)
        nlmo4 = n_elements(lumclasso4)
        indo4_1 = fltarr(nlmo4)
        indo4_2 = indo4_1
        indo4_3 = indo4_1
        indo4_4 = indo4_1 
        countindo4_1 = indo4_1
        countindo4_2 = indo4_1
        countindo4_3 = indo4_1
        countindo4_4 = indo4_1
        FOR i=0L,nlmo4-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo4_1[i] =  where(testo4 and params EQ 1, countindo4_1x); index of radius of this stellar population in the val array
            countindo4_1[i] = countindo4_1x
            indo4_2[i] =  where(testo4 and params EQ 2, countindo4_2x); index of temperature of this stellar population in the val array
            countindo4_2[i] = countindo4_2x
            indo4_3[i] =  where(testo4 and params EQ 3, countindo4_3x); index of distance of this stellar population in the val array
            countindo4_3[i] = countindo4_3x
            indo4_4[i] =  where(testo4 and params EQ 4, countindo4_4x); index of the nstars of this stellar population in the val array
            countindo4_4[i] = countindo4_4x
        ENDFOR

    ENDIF
    
    ; Locating the O5 stellar population parameters

    testo5 = strupcase(strmid(key,0,2)) EQ 'O5' 

    ind = where(testo5,countindo5)

    
    ; retrieveing the defaut values from the txt database
    tsto5 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O5' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto5,ctdato5)
    if ctdato5 ne 0 then begin
        
        T_eff_MS_o5 = double(T_eff_MS(indat))
        R_star_MS_o5 = double(R_star_MS(indat))
        
    endif

    IF countindo5 NE 0 THEN BEGIN

        lumclasso5 = lumclass(ind)
        nlmo5 = n_elements(lumclasso5)
        indo5_1 = fltarr(nlmo5)
        indo5_2 = indo5_1
        indo5_3 = indo5_1
        indo5_4 = indo5_1   
        countindo5_1 = indo5_1
        countindo5_2 = indo5_1
        countindo5_3 = indo5_1
        countindo5_4 = indo5_1
        FOR i=0L,nlmo5-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo5_1[i] =  where(testo5 and params EQ 1, countindo5_1x); index of radius of this stellar population in the val array
            countindo5_1[i] = countindo5_1x
            indo5_2[i] =  where(testo5 and params EQ 2, countindo5_2x); index of temperature of this stellar population in the val array
            countindo5_2[i] = countindo5_2x
            indo5_3[i] =  where(testo5 and params EQ 3, countindo5_3x); index of distance of this stellar population in the val array
            countindo5_3[i] = countindo5_3x
            indo5_4[i] =  where(testo5 and params EQ 4, countindo5_4x); index of the nstars of this stellar population in the val array
            countindo5_4[i] = countindo5_4x
        ENDFOR

    ENDIF
    
    ; Locating the O6 stellar population parameters

    testo6 = strupcase(strmid(key,0,2)) EQ 'O6'

    ind = where(testo6,countindo6)

    ; retrieveing the defaut values from the txt database
    tsto6 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O6' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto6,ctdato6)
    if ctdato6 ne 0 then begin
        
        T_eff_MS_o6 = double(T_eff_MS(indat))
        R_star_MS_o6 = double(R_star_MS(indat))
        
    endif

    IF countindo6 NE 0 THEN BEGIN

        lumclasso6 = lumclass(ind)
        nlmo6 = long(n_elements(lumclasso6))
        indo6_1 = fltarr(nlmo6)
        indo6_2 = indo6_1
        indo6_3 = indo6_1
        indo6_4 = indo6_1    
        countindo6_1 = indo6_1
        countindo6_2 = indo6_1
        countindo6_3 = indo6_1
        countindo6_4 = indo6_1
        FOR i=0L,nlmo6-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo6_1[i] =  where(testo6 and params EQ 1, countindo6_1x); index of radius of this stellar population in the val array
            countindo6_1[i] = countindo6_1x
            indo6_2[i] =  where(testo6 and params EQ 2, countindo6_2x); index of temperature of this stellar population in the val array
            countindo6_2[i] = countindo6_2x
            indo6_3[i] =  where(testo6 and params EQ 3, countindo6_3x); index of distance of this stellar population in the val array
            countindo6_3[i] = countindo6_3x
            indo6_4[i] =  where(testo6 and params EQ 4, countindo6_4x); index of the nstars of this stellar population in the val array
            countindo6_4[i] = countindo6_4x
        ENDFOR

    ENDIF
    

    ; Locating the O7 stellar population parameters

    testo7 = strupcase(strmid(key,0,2)) EQ 'O7' 

    ind = where(testo7,countindo7)

    ; retrieveing the defaut values from the txt database
    tsto7 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O7' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto7,ctdato7)
    if ctdato7 ne 0 then begin
        
        T_eff_MS_o7 = double(T_eff_MS(indat))
        R_star_MS_o7 = double(R_star_MS(indat))
        
    endif

    IF countindo7 NE 0 THEN BEGIN

        lumclasso7 = lumclass(ind)
        nlmo7 = n_elements(lumclasso7)
        indo7_1 = fltarr(nlmo7)
        indo7_2 = indo7_1
        indo7_3 = indo7_1
        indo7_4 = indo7_1    
        countindo7_1 = indo7_1
        countindo7_2 = indo7_1
        countindo7_3 = indo7_1
        countindo7_4 = indo7_1
        FOR i=0L,nlmo7-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo7_1[i] =  where(testo7 and params EQ 1, countindo7_1x); index of radius of this stellar population in the val array
            countindo7_1[i] = countindo7_1x
            indo7_2[i] =  where(testo7 and params EQ 2, countindo7_2x); index of temperature of this stellar population in the val array
            countindo7_2[i] = countindo7_2x
            indo7_3[i] =  where(testo7 and params EQ 3, countindo7_3x); index of distance of this stellar population in the val array
            countindo7_3[i] = countindo7_3x
            indo7_4[i] =  where(testo7 and params EQ 4, countindo7_4x); index of the nstars of this stellar population in the val array
            countindo7_4[i] = countindo7_4x
        ENDFOR

    ENDIF
    
    ; Locating the O8 stellar population parameters

    testo8 = strupcase(strmid(key,0,2)) EQ 'O8' 

    ind = where(testo8,countindo8)

    ; retrieveing the defaut values from the txt database
    tsto8 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O8' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto8,ctdato8)
    if ctdato8 ne 0 then begin
        
        T_eff_MS_o8 = double(T_eff_MS(indat))
        R_star_MS_o8 = double(R_star_MS(indat))
        
    endif

    IF countindo8 NE 0 THEN BEGIN

        lumclasso8 = lumclass(ind)
        nlmo8 = n_elements(lumclasso8)
        indo8_1 = fltarr(nlmo8)
        indo8_2 = indo8_1
        indo8_3 = indo8_1
        indo8_4 = indo8_1   
        countindo8_1 = indo8_1
        countindo8_2 = indo8_1
        countindo8_3 = indo8_1
        countindo8_4 = indo8_1
        FOR i=0L,nlmo8-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo8_1[i] =  where(testo8 and params EQ 1, countindo8_1x); index of radius of this stellar population in the val array
            countindo8_1[i] = countindo8_1x
            indo8_2[i] =  where(testo8 and params EQ 2, countindo8_2x); index of temperature of this stellar population in the val array
            countindo8_2[i] = countindo8_2x
            indo8_3[i] =  where(testo8 and params EQ 3, countindo8_3x); index of distance of this stellar population in the val array
            countindo8_3[i] = countindo8_3x
            indo8_4[i] =  where(testo8 and params EQ 4, countindo8_4x); index of the nstars of this stellar population in the val array
            countindo8_4[i] = countindo8_4x
        ENDFOR

    ENDIF
    
    ; Locating the O9 stellar population parameters

    testo9 = strupcase(strmid(key,0,2)) EQ 'O9' 

    ind = where(testo9,countindo9)

    ; retrieveing the defaut values from the txt database
    tsto9 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'O9' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsto9,ctdato9)
    if ctdato9 ne 0 then begin
        
        T_eff_MS_o9 = double(T_eff_MS(indat))
        R_star_MS_o9 = double(R_star_MS(indat))
        
    endif

    IF countindo9 NE 0 THEN BEGIN

        lumclasso9 = strupcase(lumclass(ind))
        nlmo9 = long(n_elements(lumclasso9))
        indo9_1 = fltarr(nlmo9)
        indo9_2 = indo9_1 
        indo9_3 = indo9_1 
        indo9_4 = indo9_1    
        countindo9_1 = indo9_1 
        countindo9_2 = indo9_1 
        countindo9_3 = indo9_1 
        countindo9_4 = indo9_1  
        FOR i=0L,nlmo9-1 DO BEGIN
            popnumber+=1
            counto+=1
            indo9_1[i] =  where(testo9 and params EQ 1, countindo9_1x); index of radius of this stellar population in the val array
            countindo9_1[i] = countindo9_1x
            indo9_2[i] =  where(testo9 and params EQ 2, countindo9_2x); index of temperature of this stellar population in the val array
            countindo9_2[i] = countindo9_2x
            indo9_3[i] =  where(testo9 and params EQ 3, countindo9_3x); index of distance of this stellar population in the val array
            countindo9_3[i] = countindo9_3x
            indo9_4[i] =  where(testo9 and params EQ 4, countindo9_4x); index of the nstars of this stellar population in the val array
            countindo9_4[i] = countindo9_4x
        ENDFOR

    ENDIF
    
    ;======================================================
    
    ; Locating the B0 stellar population parameters

    testb0 = strupcase(strmid(key,0,2)) EQ 'B0' 

    ind = where(testb0,countindb0)

    ; retrieveing the defaut values from the txt database
    tstb0 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B0' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb0,ctdatb0)
    if ctdatb0 ne 0 then begin
        
        T_eff_MS_b0 = double(T_eff_MS(indat))
        R_star_MS_b0 = double(R_star_MS(indat))
        
    endif

    IF countindb0 NE 0 THEN BEGIN

         lumclassb0 = uniq(lumclass(ind))
         nlmb0 = n_elements(lumclassb0)
         indb0_1 = fltarr(nlmb0)
         indb0_2 = indb0_1
         indb0_3 = indb0_1
         indb0_4 = indb0_1  
         countindb0_1 = indb0_1
         countindb0_2 = indb0_1
         countindb0_3 = indb0_1
         countindb0_4 = indb0_1       
         FOR i=0L,nlmb0-1 DO BEGIN   
            popnumber+=1
            countb+=1
            indb0_1[i] =  where(testb0 and params EQ 1, countindb0_1x); index of radius of this stellar population in the val array
            countindb0_1[i] = countindb0_1x
            indb0_2[i] =  where(testb0 and params EQ 2, countindb0_2x); index of temperature of this stellar population in the val array
            countindb0_2[i] = countindb0_2x
            indb0_3[i] =  where(testb0 and params EQ 3, countindb0_3x); index of distance of this stellar population in the val array
            countindb0_3[i] = countindb0_3x
            indb0_4[i] =  where(testb0 and params EQ 4, countindb0_4x); index of the nstars of this stellar population in the val array
            countindb0_4[i] = countindb0_4x
        ENDFOR

    ENDIF
    
    ; Locating the B1 stellar population parameters

    testb1 = strupcase(strmid(key,0,2)) EQ 'B1' 

    ind = where(testb1,countindb1)

    ; retrieveing the defaut values from the txt database
    tstb1 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B1' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb1,ctdatb1)
    if ctdatb1 ne 0 then begin
        
        T_eff_MS_b1 = double(T_eff_MS(indat))
        R_star_MS_b1 = double(R_star_MS(indat))
        
    endif

    IF countindb1 NE 0 THEN BEGIN

        lumclassb1 = strupcase(lumclass(ind))
        nlmb1 = long(n_elements(lumclassb1))
        indb1_1 = fltarr(nlmb1)
        indb1_2 = indb1_1
        indb1_3 = indb1_1
        indb1_4 = indb1_1 
        countindb1_1 = indb1_1
        countindb1_2 = indb1_1
        countindb1_3 = indb1_1
        countindb1_4 = indb1_1     
        FOR i=0L,nlmb1-1 DO BEGIN 
            popnumber+=1
            countb+=1
            indb1_1[i] =  where(testb1 and params EQ 1, countindb1_1x); index of radius of this stellar population in the val array
            countindb1_1[i] = countindb1_1x
            indb1_2[i] =  where(testb1 and params EQ 2, countindb1_2x); index of temperature of this stellar population in the val array
            countindb1_2[i] = countindb1_2x
            indb1_3[i] =  where(testb1 and params EQ 3, countindb1_3x); index of distance of this stellar population in the val array
            countindb1_3[i] = countindb1_3x
            indb1_4[i] =  where(testb1 and params EQ 4, countindb1_4x); index of the nstars of this stellar population in the val array
            countindb1_4[i] = countindb1_4x
        ENDFOR

    ENDIF
    
    ; Locating the B2 stellar population parameters

    testb2 = strupcase(strmid(key,0,2)) EQ 'B2' 

    ind = where(testb2,countindb2)

    ; retrieveing the defaut values from the txt database
    tstb2 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B2' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb2,ctdatb2)
    if ctdatb2 ne 0 then begin
        
        T_eff_MS_b2 = double(T_eff_MS(indat))
        R_star_MS_b2 = double(R_star_MS(indat))
        
    endif

    IF countindb2 NE 0 THEN BEGIN

        lumclassb2 = uniq(lumclass(ind))
        nlmb2 = n_elements(lumclassb2)
        indb2_1 = fltarr(nlmb2)
        indb2_2 = indb2_1
        indb2_3 = indb2_1
        indb2_4 = indb2_1    
        countindb2_1 = indb2_1
        countindb2_2 = indb2_1
        countindb2_3 = indb2_1
        countindb2_4 = indb2_1
        FOR i=0L,nlmb2-1 DO BEGIN 
            popnumber+=1
            countb+=1
            indb2_1[i] =  where(testb2 and params EQ 1, countindb2_1x); index of radius of this stellar population in the val array
            countindb2_1[i] = countindb2_1x
            indb2_2[i] =  where(testb2 and params EQ 2, countindb2_2x); index of temperature of this stellar population in the val array
            countindb2_2[i] = countindb2_2x
            indb2_3[i] =  where(testb2 and params EQ 3, countindb2_3x); index of distance of this stellar population in the val array
            countindb2_3[i] = countindb2_3x
            indb2_4[i] =  where(testb2 and params EQ 4, countindb2_4x); index of the nstars of this stellar population in the val array
            countindb2_4[i] = countindb2_4x
        ENDFOR

    ENDIF
    
    ; Locating the B3 stellar population parameters

    testb3 = strupcase(strmid(key,0,2)) EQ 'B3' 

    ind = where(testb3,countindb3)

    ; retrieveing the defaut values from the txt database
    tstb3 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B3' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb3,ctdatb3)
    if ctdatb3 ne 0 then begin
        
        T_eff_MS_b3 = double(T_eff_MS(indat))
        R_star_MS_b3 = double(R_star_MS(indat))
        
    endif

    IF countindb3 NE 0 THEN BEGIN

        lumclassb3 = uniq(lumclass(ind))
        nlmb3 = n_elements(lumclassb3)
        indb3_1 = fltarr(nlmb3)
        indb3_2 = indb3_1
        indb3_3 = indb3_1
        indb3_4 = indb3_1
        countindb3_1 = indb3_1
        countindb3_2 = indb3_1
        countindb3_3 = indb3_1
        countindb3_4 = indb3_1
        FOR i=0L,nlmb3-1 DO BEGIN 
            popnumber+=1
            countb+=1
            indb3_1[i] =  where(testb3 and params EQ 1, countindb3_1x); index of radius of this stellar population in the val array
            countindb3_1[i] = countindb3_1x
            indb3_2[i] =  where(testb3 and params EQ 2, countindb3_2x); index of temperature of this stellar population in the val array
            countindb3_2[i] = countindb3_2x
            indb3_3[i] =  where(testb3 and params EQ 3, countindb3_3x); index of distance of this stellar population in the val array
            countindb3_3[i] = countindb3_3x
            indb3_4[i] =  where(testb3 and params EQ 4, countindb3_4x); index of the nstars of this stellar population in the val array
            countindb3_4[i] = countindb3_4x
        ENDFOR

    ENDIF
    
    ; Locating the B4 stellar population parameters

    testb4 = strupcase(strmid(key,0,2)) EQ 'B4' 

    ind = where(testb4,countindb4)

    ; retrieveing the defaut values from the txt database
    tstb4 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B4' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb4,ctdatb4)
    if ctdatb4 ne 0 then begin
        
        T_eff_MS_b4 = double(T_eff_MS(indat))
        R_star_MS_b4 = double(R_star_MS(indat))
        
    endif

    IF countindb4 NE 0 THEN BEGIN

        lumclassb4 = uniq(lumclass(ind))
        nlmb4 = n_elements(lumclassb4)
        indb4_1 = fltarr(nlmb4)
        indb4_2 = indb4_1
        indb4_3 = indb4_1
        indb4_4 = indb4_1
        countindb4_1 = indb4_1
        countindb4_2 = indb4_1
        countindb4_3 = indb4_1
        countindb4_4 = indb4_1
        FOR i=0L,nlmb4-1 DO BEGIN 
            popnumber+=1
            countb+=1
            indb4_1[i] =  where(testb4 and params EQ 1, countindb4_1x); index of radius of this stellar population in the val array
            countindb4_1[i] = countindb4_1x
            indb4_2[i] =  where(testb4 and params EQ 2, countindb4_2x); index of temperature of this stellar population in the val array
            countindb4_2[i] = countindb4_2x
            indb4_3[i] =  where(testb4 and params EQ 3, countindb4_3x); index of distance of this stellar population in the val array
            countindb4_3[i] = countindb4_3x
            indb4_4[i] =  where(testb4 and params EQ 4, countindb4_4x); index of the nstars of this stellar population in the val array
            countindb4_4[i] = countindb4_4x
        ENDFOR

    ENDIF
    
    ; Locating the B5 stellar population parameters

    testb5 = strupcase(strmid(key,0,2)) EQ 'B5' 

    ind = where(testb5,countindb5)

    ; retrieveing the defaut values from the txt database
    tstb5 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B5' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb5,ctdatb5)
    if ctdatb5 ne 0 then begin
        
        T_eff_MS_b5 = double(T_eff_MS(indat))
        R_star_MS_b5 = double(R_star_MS(indat))
        
    endif

    IF countindb5 NE 0 THEN BEGIN

        lumclassb5 = uniq(lumclass(ind))
        nlmb5 = n_elements(lumclassb5)
        indb5_1 = fltarr(nlmb5)
        indb5_2 = indb5_1
        indb5_3 = indb5_1
        indb5_4 = indb5_1
        countindb5_1 = indb5_1
        countindb5_2 = indb5_1
        countindb5_3 = indb5_1
        countindb5_4 = indb5_1
        FOR i=0L,nlmb5-1 DO BEGIN    
            popnumber+=1
            countb+=1
            indb5_1[i] =  where(testb5 and params EQ 1, countindb5_1x); index of radius of this stellar population in the val array
            countindb5_1[i] = countindb5_1x
            indb5_2[i] =  where(testb5 and params EQ 2, countindb5_2x); index of temperature of this stellar population in the val array
            countindb5_2[i] = countindb5_2x
            indb5_3[i] =  where(testb5 and params EQ 3, countindb5_3x); index of distance of this stellar population in the val array
            countindb5_3[i] = countindb5_3x
            indb5_4[i] =  where(testb5 and params EQ 4, countindb5_4x); index of the nstars of this stellar population in the val array
            countindb5_4[i] = countindb5_4x
        ENDFOR

    ENDIF
    
    ; Locating the B6 stellar population parameters

    testb6 = strupcase(strmid(key,0,2)) EQ 'B6'

    ind = where(testb6,countindb6)

    ; retrieveing the defaut values from the txt database
    tstb6 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B6' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb6,ctdatb6)
    if ctdatb6 ne 0 then begin
        
        T_eff_MS_b6 = double(T_eff_MS(indat))
        R_star_MS_b6 = double(R_star_MS(indat))
        
    endif

    IF countindb6 NE 0 THEN BEGIN

        lumclassb6 = uniq(lumclass(ind))
        nlmb6 = n_elements(lumclassb6)
        indb6_1 = fltarr(nlmb6)
        indb6_2 = indb6_1
        indb6_3 = indb6_1
        indb6_4 = indb6_1
        countindb6_1 = indb6_1
        countindb6_2 = indb6_1
        countindb6_3 = indb6_1
        countindb6_4 = indb6_1
        FOR i=0L,nlmb6-1 DO BEGIN 
            popnumber+=1
            countb+=1
            indb6_1[i] =  where(testb6 and params EQ 1, countindb6_1x); index of radius of this stellar population in the val array
            countindb6_1[i] = countindb6_1x
            indb6_2[i] =  where(testb6 and params EQ 2, countindb6_2x); index of temperature of this stellar population in the val array
            countindb6_2[i] = countindb6_2x
            indb6_3[i] =  where(testb6 and params EQ 3, countindb6_3x); index of distance of this stellar population in the val array
            countindb6_3[i] = countindb6_3x
            indb6_4[i] =  where(testb6 and params EQ 4, countindb6_4x); index of the nstars of this stellar population in the val array
            countindb6_4[i] = countindb6_4x
        ENDFOR

    ENDIF
    
    ; Locating the B7 stellar population parameters

    testb7 = strupcase(strmid(key,0,2)) EQ 'B7' 

    ind = where(testb7,countindb7)

    ; retrieveing the defaut values from the txt database
    tstb7 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B7' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb7,ctdatb7)
    if ctdatb7 ne 0 then begin
        
        T_eff_MS_b7 = double(T_eff_MS(indat))
        R_star_MS_b7 = double(R_star_MS(indat))
        
    endif

    IF countindb7 NE 0 THEN BEGIN

        lumclassb7 = uniq(lumclass(ind))
        nlmb7 = n_elements(lumclassb7)
        indb7_1 = fltarr(nlmb7)
        indb7_2 = indb7_1
        indb7_3 = indb7_1
        indb7_4 = indb7_1  
        countindb7_1 = indb7_1
        countindb7_2 = indb7_1
        countindb7_3 = indb7_1
        countindb7_4 = indb7_1
        FOR i=0L,nlmb7-1 DO BEGIN 
            popnumber+=1
            countb+=1
            indb7_1[i] =  where(testb7 and params EQ 1, countindb7_1x); index of radius of this stellar population in the val array
            countindb7_1[i] = countindb7_1x
            indb7_2[i] =  where(testb7 and params EQ 2, countindb7_2x); index of temperature of this stellar population in the val array
            countindb7_2[i] = countindb7_2x
            indb7_3[i] =  where(testb7 and params EQ 3, countindb7_3x); index of distance of this stellar population in the val array
            countindb7_3[i] = countindb7_3x
            indb7_4[i] =  where(testb7 and params EQ 4, countindb7_4x); index of the nstars of this stellar population in the val array
            countindb7_4[i] = countindb7_4x
        ENDFOR

    ENDIF
    
    ; Locating the B8 stellar population parameters

    testb8 = strupcase(strmid(key,0,2)) EQ 'B8'  

    ind = where(testb8,countindb8)

    ; retrieveing the defaut values from the txt database
    tstb8 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B8' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb8,ctdatb8)
    if ctdatb8 ne 0 then begin
        
        T_eff_MS_b8 = double(T_eff_MS(indat))
        R_star_MS_b8 = double(R_star_MS(indat))
        
    endif

    IF countindb8 NE 0 THEN BEGIN

        lumclassb8 = uniq(lumclass(ind))
        nlmb8 = n_elements(lumclassb8)
        indb8_1 = fltarr(nlmb8)
        indb8_2 = indb8_1
        indb8_3 = indb8_1
        indb8_4 = indb8_1   
        countindb8_1 = indb8_1
        countindb8_2 = indb8_1
        countindb8_3 = indb8_1
        countindb8_4 = indb8_1
        FOR i=0L,nlmb8-1 DO BEGIN
            popnumber+=1
            countb+=1
            indb8_1[i] =  where(testb8 and params EQ 1, countindb8_1x); index of radius of this stellar population in the val array
            countindb8_1[i] = countindb8_1x
            indb8_2[i] =  where(testb8 and params EQ 2, countindb8_2x); index of temperature of this stellar population in the val array
            countindb8_2[i] = countindb8_2x
            indb8_3[i] =  where(testb8 and params EQ 3, countindb8_3x); index of distance of this stellar population in the val array
            countindb8_3[i] = countindb8_3x
            indb8_4[i] =  where(testb8 and params EQ 4, countindb8_4x); index of the nstars of this stellar population in the val array
            countindb8_4[i] = countindb8_4x
        ENDFOR

    ENDIF
    
    ; Locating the B9 stellar population parameters

    testb9 = strupcase(strmid(key,0,2)) EQ 'B9' 

    ind = where(testb9,countindb9)

    ; retrieveing the defaut values from the txt database
    tstb9 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'B9' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstb9,ctdatb9)
    if ctdatb9 ne 0 then begin
        
        T_eff_MS_b9 = double(T_eff_MS(indat))
        R_star_MS_b9 = double(R_star_MS(indat))
        
    endif

    IF countindb9 NE 0 THEN BEGIN

        lumclassb9 = uniq(lumclass(ind))
        nlmb9 = n_elements(lumclassb9)
        indb9_1 = fltarr(nlmb9)
        indb9_2 = indb9_1
        indb9_3 = indb9_1
        indb9_4 = indb9_1   
        countindb9_1 = indb9_1
        countindb9_2 = indb9_1
        countindb9_3 = indb9_1
        countindb9_4 = indb9_1
        FOR i=0L,nlmb9-1 DO BEGIN
            popnumber+=1
            countb+=1
            indb9_1[i] =  where(testb9 and params EQ 1, countindb9_1x); index of radius of this stellar population in the val array
            countindb9_1[i] = countindb9_1x
            indb9_2[i] =  where(testb9 and params EQ 2, countindb9_2x); index of temperature of this stellar population in the val array
            countindb9_2[i] = countindb9_2x
            indb9_3[i] =  where(testb9 and params EQ 3, countindb9_3x); index of distance of this stellar population in the val array
            countindb9_3[i] = countindb9_3x
            indb9_4[i] =  where(testb9 and params EQ 4, countindb9_4x); index of the nstars of this stellar population in the val array
            countindb9_4[i] = countindb9_4x
        ENDFOR

    ENDIF
    
    
    ;======================================================
    
    ; Locating the A0 stellar population parameters

    testa0 = strupcase(strmid(key,0,2)) EQ 'A0' 

    ind = where(testa0,countinda0)

    ; retrieveing the defaut values from the txt database
    tsta0 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A0' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsta0,ctdata0)
    if ctdata0 ne 0 then begin
        
        T_eff_MS_a0 = double(T_eff_MS(indat))
        R_star_MS_a0 = double(R_star_MS(indat))
        
    endif

    IF countinda0 NE 0 THEN BEGIN

        lumclassA0 = uniq(lumclass(ind))
        nlmA0 = n_elements(lumclassA0)
        indA0_1 = fltarr(nlmA0)
        indA0_2 = indA0_1 
        indA0_3 = indA0_1 
        indA0_4 = indA0_1    
        countindA0_1 = indA0_1 
        countindA0_2 = indA0_1 
        countindA0_3 = indA0_1 
        countindA0_4 = indA0_1  
        FOR i=0L,nlmA0-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda0_1[i] =  where(testa0 and params EQ 1, countinda0_1x); index of radius of this stellar population in the val array
            countinda0_1[i] = countinda0_1x
            inda0_2[i] =  where(testa0 and params EQ 2, countinda0_2x); index of temperature of this stellar population in the val array
            countinda0_2[i] = countinda0_2x
            inda0_3[i] =  where(testa0 and params EQ 3, countinda0_3x); index of distance of this stellar population in the val array
            countinda0_3[i] = countinda0_3x
            inda0_4[i] =  where(testa0 and params EQ 4, countinda0_4x); index of the nstars of this stellar population in the val array
            countinda0_4[i] =  countinda0_4x
        ENDFOR

    ENDIF
    
    ; Locating the A1 stellar population parameters

    testa1 = strupcase(strmid(key,0,2)) EQ 'A1' 

    ind = where(testa1,countinda1)

     ; retrieveing the defaut values from the txt database
     tsta1 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A1' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
     indat  = where(tsta1,ctdata1)
     if ctdata1 ne 0 then begin
         
         T_eff_MS_a1 = double(T_eff_MS(indat))
         R_star_MS_a1 = double(R_star_MS(indat))
         
     endif
     

    IF countinda1 NE 0 THEN BEGIN

        lumclassA1 = lumclass(ind)
        nlmA1 = n_elements(lumclassA1)
        indA1_1 = fltarr(nlmA1)
        indA1_2 = indA1_1
        indA1_3 = indA1_1
        indA1_4 = indA1_1  
        countindA1_1 = indA1_1
        countindA1_2 = indA1_1
        countindA1_3 = indA1_1
        countindA1_4 = indA1_1
        FOR i=0L,nlmA1-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda1_1[i] =  where(testa1 and params EQ 1, countinda1_1x); index of radius of this stellar population in the val array
            countinda1_1[i] = countinda1_1x
            inda1_2[i] =  where(testa1 and params EQ 2, countinda1_2x); index of temperature of this stellar population in the val array
            countinda1_2[i] = countinda1_2x
            inda1_3[i] =  where(testa1 and params EQ 3, countinda1_3x); index of distance of this stellar population in the val array
            countinda1_3[i] = countinda1_3x
            inda1_4[i] =  where(testa1 and params EQ 4, countinda1_4x); index of the nstars of this stellar population in the val array
            countinda1_4[i] = countinda1_4x
        ENDFOR

    ENDIF
    
    ; Locating the A2 stellar population parameters

    testa2 = strupcase(strmid(key,0,2)) EQ 'A2' 

    ind = where(testa2,countinda2)

     ; retrieveing the defaut values from the txt database
     tsta2 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A2' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
     indat  = where(tsta2,ctdata2)
     if ctdata2 ne 0 then begin
         
         T_eff_MS_a2 = double(T_eff_MS(indat))
         R_star_MS_a2 = double(R_star_MS(indat))
         
     endif

    IF countinda2 NE 0 THEN BEGIN

        lumclassA2 = lumclass(ind)
        nlmA2 = n_elements(lumclassA2)
        indA2_1 = fltarr(nlmA2)
        indA2_2 = indA2_1
        indA2_3 = indA2_1
        indA2_4 = indA2_1
        countindA2_1 = indA2_1
        countindA2_2 = indA2_1
        countindA2_3 = indA2_1
        countindA2_4 = indA2_1
        FOR i=0L,nlmA2-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda2_1[i] =  where(testa2 and params EQ 1, countinda2_1x); index of radius of this stellar population in the val array
            countinda2_1[i] = countinda2_1x
            inda2_2[i] =  where(testa2 and params EQ 2, countinda2_2x); index of temperature of this stellar population in the val array
            countinda2_2[i] = countinda2_2x
            inda2_3[i] =  where(testa2 and params EQ 3, countinda2_3x); index of distance of this stellar population in the val array
            countinda2_3[i] = countinda2_3x
            inda2_4[i] =  where(testa2 and params EQ 4, countinda2_4x); index of the nstars of this stellar population in the val array
            countinda2_4[i] = countinda2_4x
        ENDFOR

    ENDIF
    
    ; Locating the A3 stellar population parameters

    testa3 = strupcase(strmid(key,0,2)) EQ 'A3' 

    ind = where(testa3,countinda3)

     ; retrieveing the defaut values from the txt database
     tsta3 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A3' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
     indat  = where(tsta3,ctdata3)
     if ctdata3 ne 0 then begin
         
         T_eff_MS_a3 = double(T_eff_MS(indat))
         R_star_MS_a3 = double(R_star_MS(indat))
         
     endif

    IF countinda3 NE 0 THEN BEGIN

        lumclassA3 = lumclass(ind)
        nlmA3 = n_elements(lumclassA3)
        indA3_1 = fltarr(nlmA3)
        indA3_2 = indA3_1
        indA3_3 = indA3_1
        indA3_4 = indA3_1    
        countindA3_1 = indA3_1
        countindA3_2 = indA3_1
        countindA3_3 = indA3_1
        countindA3_4 = indA3_1
        FOR i=0L,nlmA3-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda3_1[i] =  where(testa3 and params EQ 1, countinda3_1x); index of radius of this stellar population in the val array
            countinda3_1[i] = countinda3_1x
            inda3_2[i] =  where(testa3 and params EQ 2, countinda3_2x); index of temperature of this stellar population in the val array
            countinda3_2[i] = countinda3_2x
            inda3_3[i] =  where(testa3 and params EQ 3, countinda3_3x); index of distance of this stellar population in the val array
            countinda3_3[i] = countinda3_3x
            inda3_4[i] =  where(testa3 and params EQ 4, countinda3_4x); index of the nstars of this stellar population in the val array
            countinda3_4[i] = countinda3_4x
        ENDFOR

    ENDIF
    
    ; Locating the A4 stellar population parameters

    testa4 = strupcase(strmid(key,0,2)) EQ 'A4' 

    ind = where(testa4,countinda4)

     ; retrieveing the defaut values from the txt database
     tsta4 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A4' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
     indat  = where(tsta4,ctdata4)
     if ctdata4 ne 0 then begin
         
         T_eff_MS_a4 = double(T_eff_MS(indat))
         R_star_MS_a4 = double(R_star_MS(indat))
         
     endif

    IF countinda4 NE 0 THEN BEGIN

        lumclassA4 = lumclass(ind)
        nlmA4 = n_elements(lumclassA4)
        indA4_1 = fltarr(nlmA4)
        indA4_2 = indA4_1
        indA4_3 = indA4_1
        indA4_4 = indA4_1   
        countindA4_1 = indA4_1
        countindA4_2 = indA4_1
        countindA4_3 = indA4_1
        countindA4_4 = indA4_1
        FOR i=0L,nlmA4-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda4_1[i] =  where(testa4 and params EQ 1, countinda4_1x); index of radius of this stellar population in the val array
            countinda4_1[i] = countinda4_1x
            inda4_2[i] =  where(testa4 and params EQ 2, countinda4_2x); index of temperature of this stellar population in the val array
            countinda4_2[i] = countinda4_2x
            inda4_3[i] =  where(testa4 and params EQ 3, countinda4_3x); index of distance of this stellar population in the val array
            countinda4_3[i] = countinda4_3x
            inda4_4[i] =  where(testa4 and params EQ 4, countinda4_4x); index of the nstars of this stellar population in the val array
            countinda4_4[i] = countinda4_4x
        ENDFOR

    ENDIF
    
    ; Locating the A5 stellar population parameters

    testa5 = strupcase(strmid(key,0,2)) EQ 'A5' 

    ind = where(testa5,countinda5)

     ; retrieveing the defaut values from the txt database
     tsta5 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A5' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
     indat  = where(tsta5,ctdata5)
     if ctdata5 ne 0 then begin
         
         T_eff_MS_a5 = double(T_eff_MS(indat))
         R_star_MS_a5 = double(R_star_MS(indat))
         
     endif

    IF countinda5 NE 0 THEN BEGIN

        lumclassA5 = lumclass(ind)
        nlmA5 = n_elements(lumclassA5)
        indA5_1 = fltarr(nlmA5)
        indA5_2 = indA5_1
        indA5_3 = indA5_1
        indA5_4 = indA5_1   
        countindA5_1 = indA5_1
        countindA5_2 = indA5_1
        countindA5_3 = indA5_1
        countindA5_4 = indA5_1
        FOR i=0L,nlmA5-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda5_1[i] =  where(testa5 and params EQ 1, countinda5_1x); index of radius of this stellar population in the val array
            countinda5_1[i] = countinda5_1x
            inda5_2[i] =  where(testa5 and params EQ 2, countinda5_2x); index of temperature of this stellar population in the val array
            countinda5_2[i] = countinda5_2x
            inda5_3[i] =  where(testa5 and params EQ 3, countinda5_3x); index of distance of this stellar population in the val array
            countinda5_3[i] = countinda5_3x
            inda5_4[i] =  where(testa5 and params EQ 4, countinda5_4x); index of the nstars of this stellar population in the val array
            countinda5_4[i] = countinda5_4x
        ENDFOR

    ENDIF
    
    ; Locating the A6 stellar population parameters

    testa6 = strupcase(strmid(key,0,2)) EQ 'A6'

    ind = where(testa6,countinda6)

     ; retrieveing the defaut values from the txt database
     tsta6 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A6' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
     indat  = where(tsta6,ctdata6)
     if ctdata6 ne 0 then begin
         
         T_eff_MS_a6 = double(T_eff_MS(indat))
         R_star_MS_a6 = double(R_star_MS(indat))
         
     endif

    IF countinda6 NE 0 THEN BEGIN

        lumclassA6 = lumclass(ind)
        nlmA6 = n_elements(lumclassA6)
        indA6_1 = fltarr(nlmA6)
        indA6_2 = indA6_1
        indA6_3 = indA6_1
        indA6_4 = indA6_1   
        countindA6_1 = indA6_1
        countindA6_2 = indA6_1
        countindA6_3 = indA6_1
        countindA6_4 = indA6_1
        FOR i=0L,nlmA6-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda6_1[i] =  where(testa6 and params EQ 1, countinda6_1x); index of radius of this stellar population in the val array
            countinda6_1[i] = countinda6_1x
            inda6_2[i] =  where(testa6 and params EQ 2, countinda6_2x); index of temperature of this stellar population in the val array
            countinda6_2[i] = countinda6_2x
            inda6_3[i] =  where(testa6 and params EQ 3, countinda6_3x); index of distance of this stellar population in the val array
            countinda6_3[i] = countinda6_3x
            inda6_4[i] =  where(testa6 and params EQ 4, countinda6_4x); index of the nstars of this stellar population in the val array
            countinda6_4[i] = countinda6_4x
        ENDFOR

    ENDIF
    
    ; Locating the A7 stellar population parameters

    testa7 = strupcase(strmid(key,0,2)) EQ 'A7'

    ind = where(testa7,countinda7)

    ; retrieveing the defaut values from the txt database
    tsta7 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A7' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsta7,ctdata7)
    if ctdata7 ne 0 then begin
         
        T_eff_MS_a7 = double(T_eff_MS(indat))
        R_star_MS_a7 = double(R_star_MS(indat))
        
    endif

    IF countinda7 NE 0 THEN BEGIN

        lumclassA7 = lumclass(ind)
        nlmA7 = n_elements(lumclassA7)
        indA7_1 = fltarr(nlmA7)
        indA7_2 = indA7_1
        indA7_3 = indA7_1
        indA7_4 = indA7_1  
        countindA7_1 = indA7_1
        countindA7_2 = indA7_1
        countindA7_3 = indA7_1
        countindA7_4 = indA7_1
        FOR i=0L,nlmA7-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda7_1[i] =  where(testa7 and params EQ 1, countinda7_1x); index of radius of this stellar population in the val array
            countinda7_1[i] = countinda7_1x
            inda7_2[i] =  where(testa7 and params EQ 2, countinda7_2x); index of temperature of this stellar population in the val array
            countinda7_2[i] = countinda7_2x
            inda7_3[i] =  where(testa7 and params EQ 3, countinda7_3x); index of distance of this stellar population in the val array
            countinda7_3[i] = countinda7_3x
            inda7_4[i] =  where(testa7 and params EQ 4, countinda7_4x); index of the nstars of this stellar population in the val array
            countinda7_4[i] = countinda7_4x
       ENDFOR

    ENDIF
    
    ; Locating the A8 stellar population parameters

    testa8 = strupcase(strmid(key,0,2)) EQ 'A8'

    ind = where(testa8,countinda8)

    ; retrieveing the defaut values from the txt database
    tsta8 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A8' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsta8,ctdata8)
    if ctdata8 ne 0 then begin
         
        T_eff_MS_a8 = double(T_eff_MS(indat))
        R_star_MS_a8 = double(R_star_MS(indat))
        
    endif

    IF countinda8 NE 0 THEN BEGIN

        lumclassA8 = lumclass(ind)
        nlmA8 = n_elements(lumclassA8)
        indA8_1 = fltarr(nlmA8)
        indA8_2 = indA8_1
        indA8_3 = indA8_1
        indA8_4 = indA8_1
        countindA8_1 = indA8_1
        countindA8_2 = indA8_1
        countindA8_3 = indA8_1
        countindA8_4 = indA8_1
        FOR i=0L,nlmA8-1 DO BEGIN
            popnumber+=1
            counta+=1
            inda8_1[i] =  where(testa8 and params EQ 1, countinda8_1x); index of radius of this stellar population in the val array
            countinda8_1[i] = countinda8_1x
            inda8_2[i] =  where(testa8 and params EQ 2, countinda8_2x); index of temperature of this stellar population in the val array
            countinda8_2[i] = countinda8_2x
            inda8_3[i] =  where(testa8 and params EQ 3, countinda8_3x); index of distance of this stellar population in the val array
            countinda8_3[i] = countinda8_3x
            inda8_4[i] =  where(testa8 and params EQ 4, countinda8_4x); index of the nstars of this stellar population in the val array
            countinda8_4[i] = countinda8_4x
        ENDFOR

    ENDIF
   
    ; Locating the A9 stellar population parameters

    testa9 = strupcase(strmid(key,0,2)) EQ 'A9' 

    ind = where(testa9,countinda9)

    ; retrieveing the defaut values from the txt database
    tsta9 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'A9' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tsta9,ctdata9)
    if ctdata9 ne 0 then begin
         
        T_eff_MS_a9 = double(T_eff_MS(indat))
        R_star_MS_a9 = double(R_star_MS(indat))
        
    endif

    IF countinda9 NE 0 THEN BEGIN

        lumclassA9 = lumclass(ind)
        nlmA9 = n_elements(lumclassA9)
        indA9_1 = fltarr(nlmA9)
        indA9_2 = indA9_1
        indA9_3 = indA9_1
        indA9_4 = indA9_1    
        countindA9_1 = indA9_1
        countindA9_2 = indA9_1
        countindA9_3 = indA9_1
        countindA9_4 = indA9_1
        FOR i=0L,nlmA9-1 DO BEGIN
            popnumber+=1  
            counta+=1
            inda9_1[i] =  where(testa9 and params EQ 1, countinda9_1x); index of radius of this stellar population in the val array
            countinda9_1[i] = countinda9_1x
            inda9_2[i] =  where(testa9 and params EQ 2, countinda9_2x); index of temperature of this stellar population in the val array
            countinda9_2[i] = countinda9_2x
            inda9_3[i] =  where(testa9 and params EQ 3, countinda9_3x); index of distance of this stellar population in the val array
            countinda9_3[i] = countinda9_3x
            inda9_4[i] =  where(testa9 and params EQ 4, countinda9_4x); index of the nstars of this stellar population in the val array
            countinda9_4[i] = countinda9_4x
        ENDFOR

    ENDIF
    
    
    ;====================================================== 
     
    ; Locating the F0 stellar population parameters 

    testf0 = strupcase(strmid(key,0,2)) EQ 'F0' 

    ind = where(testf0,countindf0)

    ; retrieveing the defaut values from the txt database
    tstf0 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F0' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf0,ctdatf0)
    if ctdatf0 ne 0 then begin
         
        T_eff_MS_f0 = double(T_eff_MS(indat))
        R_star_MS_f0 = double(R_star_MS(indat))
        
    endif

    IF countindf0 NE 0 THEN BEGIN

        lumclassF0 = lumclass(ind)
        nlmF0 = n_elements(lumclassF0)
        indF0_1 = fltarr(nlmF0)
        indF0_2 = indF0_1
        indF0_3 = indF0_1
        indF0_4 = indF0_1
        countindF0_1 = indF0_1
        countindF0_2 = indF0_1
        countindF0_3 = indF0_1
        countindF0_4 = indF0_1
        FOR i=0L,nlmF0-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf0_1[i] =  where(testf0 and params EQ 1, countindf0_1x); index of radius of this stellar population in the val array
            countindf0_1[i] = countindf0_1x
            indf0_2[i] =  where(testf0 and params EQ 2, countindf0_2x); index of temperature of this stellar population in the val array
            countindf0_2[i] = countindf0_2x
            indf0_3[i] =  where(testf0 and params EQ 3, countindf0_3x); index of distance of this stellar population in the val array
            countindf0_3[i] = countindf0_3x
            indf0_4[i] =  where(testf0 and params EQ 4, countindf0_4x); index of the nstars of this stellar population in the val array
            countindf0_4[i] = countindf0_4x
        ENDFOR

    ENDIF
    
    ; Locating the F1 stellar population parameters

    testf1 = strupcase(strmid(key,0,2)) EQ 'F1' 

    ind = where(testf1,countindf1)

    ; retrieveing the defaut values from the txt database
    tstf1 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F1' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf1,ctdatf1)
    if ctdatf1 ne 0 then begin
         
        T_eff_MS_f1 = double(T_eff_MS(indat))
        R_star_MS_f1 = double(R_star_MS(indat))
        
    endif

    IF countindf1 NE 0 THEN BEGIN

        lumclassF1 = lumclass(ind)
        nlmF1 = n_elements(lumclassF1)
        indF1_1 = fltarr(nlmF1)
        indF1_2 = indF1_1
        indF1_3 = indF1_1
        indF1_4 = indF1_1
        countindF1_1 = indF1_1
        countindF1_2 = indF1_1
        countindF1_3 = indF1_1
        countindF1_4 = indF1_1
        FOR i=0L,nlmF1-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf1_1[i] =  where(testf1 and params EQ 1, countindf1_1x); index of radius of this stellar population in the val array
            countindf1_1[i] = countindf1_1x
            indf1_2[i] =  where(testf1 and params EQ 2, countindf1_2x); index of temperature of this stellar population in the val array
            countindf1_2[i] = countindf1_2x
            indf1_3[i] =  where(testf1 and params EQ 3, countindf1_3x); index of distance of this stellar population in the val array
            countindf1_3[i] = countindf1_3x
            indf1_4[i] =  where(testf1 and params EQ 4, countindf1_4x); index of the nstars of this stellar population in the val array
            countindf1_4[i] = countindf1_4x
        ENDFOR

    ENDIF
    
    ; Locating the F2 stellar population parameters

    testf2 = strupcase(strmid(key,0,2)) EQ 'F2' 

    ind = where(testf2,countindf2)

    ; retrieveing the defaut values from the txt database
    tstf2 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F2' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf2,ctdatf2)
    if ctdatf2 ne 0 then begin
         
        T_eff_MS_f2 = double(T_eff_MS(indat))
        R_star_MS_f2 = double(R_star_MS(indat))
        
    endif

    IF countindf2 NE 0 THEN BEGIN

        lumclassF2 = lumclass(ind)
        nlmF2 = n_elements(lumclassF2)
        indF2_1 = fltarr(nlmF2)
        indF2_2 = testf2
        indF2_3 = testf2
        indF2_4 = testf2
        countindF2_1 = testf2
        countindF2_2 = testf2
        countindF2_3 = testf2
        countindF2_4 = testf2
        FOR i=0L,nlmF2-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf2_1[i] =  where(testf2 and params EQ 1, countindf2_1x); index of radius of this stellar population in the val array
            countindf2_1[i] = countindf2_1x
            indf2_2[i] =  where(testf2 and params EQ 2, countindf2_2x); index of temperature of this stellar population in the val array
            countindf2_2[i] = countindf2_2x
            indf2_3[i] =  where(testf2 and params EQ 3, countindf2_3x); index of distance of this stellar population in the val array
            countindf2_3[i] = countindf2_3x
            indf2_4[i] =  where(testf2 and params EQ 4, countindf2_4x); index of the nstars of this stellar population in the val array
            countindf2_4[i] = countindf2_4x
        ENDFOR

    ENDIF
    
    ; Locating the F3 stellar population parameters

    testf3 = strupcase(strmid(key,0,2)) EQ 'F3' 

    ind = where(testf3,countindf3)

    ; retrieveing the defaut values from the txt database
    tstf3 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F3' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf3,ctdatf3)
    if ctdatf3 ne 0 then begin
         
        T_eff_MS_f3 = double(T_eff_MS(indat))
        R_star_MS_f3 = double(R_star_MS(indat))
        
    endif

    IF countindf3 NE 0 THEN BEGIN

        lumclassF3 = lumclass(ind)
        nlmF3 = n_elements(lumclassF3)
        indF3_1 = fltarr(nlmF3)
        indF3_2 = indF3_1
        indF3_3 = indF3_1
        indF3_4 = indF3_1
        countindF3_1 = indF3_1
        countindF3_2 = indF3_1
        countindF3_3 = indF3_1
        countindF3_4 = indF3_1
        FOR i=0L,nlmF3-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf3_1[i] =  where(testf3 and params EQ 1, countindf3_1x); index of radius of this stellar population in the val array
            countindf3_1[i] = countindf3_1x
            indf3_2[i] =  where(testf3 and params EQ 2, countindf3_2x); index of temperature of this stellar population in the val array
            countindf3_2[i] = countindf3_2x
            indf3_3[i] =  where(testf3 and params EQ 3, countindf3_3x); index of distance of this stellar population in the val array
            countindf3_3[i] = countindf3_3x
            indf3_4[i] =  where(testf3 and params EQ 4, countindf3_4x); index of the nstars of this stellar population in the val array
            countindf3_4[i] = countindf3_4x
        ENDFOR

    ENDIF
    
    ; Locating the F4 stellar population parameters

    testf4 = strupcase(strmid(key,0,2)) EQ 'F4'

    ind = where(testf4,countindf4)

    ; retrieveing the defaut values from the txt database
    tstf4 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F4' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf4,ctdatf4)
    if ctdatf4 ne 0 then begin
         
        T_eff_MS_f4 = double(T_eff_MS(indat))
        R_star_MS_f4 = double(R_star_MS(indat))
        
    endif

    IF countindf4 NE 0 THEN BEGIN

        lumclassF4 = lumclass(ind)
        nlmF4 = n_elements(lumclassF4)
        indF4_1 = fltarr(nlmF4)
        indF4_2 = indF4_1
        indF4_3 = indF4_1
        indF4_4 = indF4_1
        countindF4_1 = indF4_1
        countindF4_2 = indF4_1
        countindF4_3 = indF4_1
        countindF4_4 = indF4_1
        FOR i=0L,nlmF4-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf4_1[i] =  where(testf4 and params EQ 1, countindf4_1x); index of radius of this stellar population in the val array
            countindf4_1[i] = countindf4_1x
            indf4_2[i] =  where(testf4 and params EQ 2, countindf4_2x); index of temperature of this stellar population in the val array
            countindf4_2[i] = countindf4_2x
            indf4_3[i] =  where(testf4 and params EQ 3, countindf4_3x); index of distance of this stellar population in the val array
            countindf4_3[i] = countindf4_3x
            indf4_4[i] =  where(testf4 and params EQ 4, countindf4_4x); index of the nstars of this stellar population in the val array
            countindf4_4[i] = countindf4_4x
        ENDFOR

    ENDIF
    
    ; Locating the F5 stellar population parameters

    testf5 = strupcase(strmid(key,0,2)) EQ 'F5'

    ind = where(testf5,countindf5)

    ; retrieveing the defaut values from the txt database
    tstf5 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F5' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf5,ctdatf5)
    if ctdatf5 ne 0 then begin
         
        T_eff_MS_f5 = double(T_eff_MS(indat))
        R_star_MS_f5 = double(R_star_MS(indat))
        
    endif

    IF countindf5 NE 0 THEN BEGIN

       lumclassF5 = lumclass(ind)
       nlmF5 = n_elements(lumclassF5)
       indF5_1 = fltarr(nlmF5)
       indF5_2 = indF5_1
       indF5_3 = indF5_1
       indF5_4 = indF5_1
       countindF5_1 = indF5_1
       countindF5_2 = indF5_1
       countindF5_3 = indF5_1
       countindF5_4 = indF5_1
       FOR i=0L,nlmF5-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf5_1[i] =  where(testf5 and params EQ 1, countindf5_1x); index of radius of this stellar population in the val array
            countindf5_1[i] = countindf5_1x
            indf5_2[i] =  where(testf5 and params EQ 2, countindf5_2x); index of temperature of this stellar population in the val array
            countindf5_2[i] = countindf5_2x
            indf5_3[i] =  where(testf5 and params EQ 3, countindf5_3x); index of distance of this stellar population in the val array
            countindf5_3[i] = countindf5_3x
            indf5_4[i] =  where(testf5 and params EQ 4, countindf5_4x); index of the nstars of this stellar population in the val array
            countindf5_4[i] = countindf5_4x
        ENDFOR

    ENDIF
    
    ; Locating the F6 stellar population parameters

    testf6 = strupcase(strmid(key,0,2)) EQ 'F6' 

    ind = where(testf6,countindf6)

    ; retrieveing the defaut values from the txt database
    tstf6 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F6' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf6,ctdatf6)
    if ctdatf6 ne 0 then begin
         
        T_eff_MS_f6 = double(T_eff_MS(indat))
        R_star_MS_f6 = double(R_star_MS(indat))
        
    endif

    IF countindf6 NE 0 THEN BEGIN

         lumclassF6 = lumclass(ind)
         nlmF6 = n_elements(lumclassF6)
         indF6_1 = fltarr(nlmF6)
         indF6_2 = indF6_1
         indF6_3 = indF6_1
         indF6_4 = indF6_1
         countindF6_1 = indF6_1
         countindF6_2 = indF6_1
         countindF6_3 = indF6_1
         countindF6_4 = indF6_1
         FOR i=0L,nlmF6-1 DO BEGIN   
            popnumber+=1
            countf+=1
            indf6_1[i] =  where(testf6 and params EQ 1, countindf6_1x); index of radius of this stellar population in the val array
            countindf6_1[i] = countindf6_1x
            indf6_2[i] =  where(testf6 and params EQ 2, countindf6_2x); index of temperature of this stellar population in the val array
            countindf6_2[i] = countindf6_2x
            indf6_3[i] =  where(testf6 and params EQ 3, countindf6_3x); index of distance of this stellar population in the val array
            countindf6_3[i] = countindf6_3x
            indf6_4[i] =  where(testf6 and params EQ 4, countindf6_4x); index of the nstars of this stellar population in the val array
            countindf6_4[i] = countindf6_4x
         ENDFOR
     ENDIF

    
    ; Locating the F7 stellar population parameters

    testf7 = strupcase(strmid(key,0,2)) EQ 'F7' 

    ind = where(testf7,countindf7)

    ; retrieveing the defaut values from the txt database
    tstf7 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F7' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf7,ctdatf7)
    if ctdatf7 ne 0 then begin
         
        T_eff_MS_f7 = double(T_eff_MS(indat))
        R_star_MS_f7 = double(R_star_MS(indat))
        
    endif

    IF countindf7 NE 0 THEN BEGIN

        umclassF7 = lumclass(ind)
        nlmF7 = n_elements(lumclassF7)
        indF7_1 = fltarr(nlmF7)
        indF7_2 = indF7_1
        indF7_3 = indF7_1
        indF7_4 = indF7_1
        countindF7_1 = indF7_1
        countindF7_2 = indF7_1
        countindF7_3 = indF7_1
        countindF7_4 = indF7_1
        FOR i=0L,nlmF7-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf7_1[i] =  where(testf7 and params EQ 1, countindf7_1x); index of radius of this stellar population in the val array
            countindf7_1[i] = countindf7_1x
            indf7_2[i] =  where(testf7 and params EQ 2, countindf7_2x); index of temperature of this stellar population in the val array
            countindf7_2[i] = countindf7_2x
            indf7_3[i] =  where(testf7 and params EQ 3, countindf7_3x); index of distance of this stellar population in the val array
            countindf7_3[i] = countindf7_3x
            indf7_4[i] =  where(testf7 and params EQ 4, countindf7_4x); index of the nstars of this stellar population in the val array
            countindf7_4[i] = countindf7_4x
        ENDFOR

    ENDIF
    
    ; Locating the F8 stellar population parameters

    testf8 = strupcase(strmid(key,0,2)) EQ 'F8' 

    ind = where(testf8,countindf8)

    ; retrieveing the defaut values from the txt database
    tstf8 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F8' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf8,ctdatf8)
    if ctdatf8 ne 0 then begin
         
        T_eff_MS_f8 = double(T_eff_MS(indat))
        R_star_MS_f8 = double(R_star_MS(indat))
        
    endif

    IF countindf8 NE 0 THEN BEGIN

        lumclassF8 = lumclass(ind)
        nlmF8 = n_elements(lumclassF8)
        indF8_1 = fltarr(nlmF8)
        indF8_2 = indF8_1
        indF8_3 = indF8_1
        indF8_4 = indF8_1
        countindF8_1 = indF8_1
        countindF8_2 = indF8_1
        countindF8_3 = indF8_1
        countindF8_4 = indF8_1
        FOR i=0L,nlmF8-1 DO BEGIN
            popnumber+=1
            countf+=1
            indf8_1[i] =  where(testf8 and params EQ 1, countindf8_1x); index of radius of this stellar population in the val array
            countindf8_1[i] = countindf8_1x
            indf8_2[i] =  where(testf8 and params EQ 2, countindf8_2x); index of temperature of this stellar population in the val array
            countindf8_2[i] = countindf8_2x
            indf8_3[i] =  where(testf8 and params EQ 3, countindf8_3x); index of distance of this stellar population in the val array
            countindf8_3[i] = countindf8_3x
            indf8_4[i] =  where(testf8 and params EQ 4, countindf8_4x); index of the nstars of this stellar population in the val array
            countindf8_4[i] = countindf8_4x
        ENDFOR

    ENDIF
    
    ; Locating the F9 stellar population parameters

    testf9 = strupcase(strmid(key,0,2)) EQ 'F9' 

    ind = where(testf9,countindf9)

    ; retrieveing the defaut values from the txt database
    tstf9 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'F9' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstf9,ctdatf9)
    if ctdatf9 ne 0 then begin
         
        T_eff_MS_f9 = double(T_eff_MS(indat))
        R_star_MS_f9 = double(R_star_MS(indat))
        
    endif

    IF countindf9 NE 0 THEN BEGIN

        lumclassF9 = lumclass(ind)
        nlmF9 = n_elements(lumclassF9)
        indF9_1 = fltarr(nlmF9)
        indF9_2 = indF9_1
        indF9_3 = indF9_1
        indF9_4 = indF9_1
        countindF9_1 = indF9_1
        countindF9_2 = indF9_1
        countindF9_3 = indF9_1
        countindF9_4 = indF9_1
        FOR i=0L,nlmF9-1 DO BEGIN 
            popnumber+=1  
            countf+=1
            indf9_1[i] =  where(testf9 and params EQ 1, countindf9_1x); index of radius of this stellar population in the val array
            countindf9_1[i] = countindf9_1x
            indf9_2[i] =  where(testf9 and params EQ 2, countindf9_2x); index of temperature of this stellar population in the val array
            countindf9_2[i] = countindf9_2x
            indf9_3[i] =  where(testf9 and params EQ 3, countindf9_3x); index of distance of this stellar population in the val array
            countindf9_3[i] = countindf9_3x
            indf9_4[i] =  where(testf9 and params EQ 4, countindf9_4x); index of the nstars of this stellar population in the val array
            countindf9_4[i] = countindf9_4x
        ENDFOR

    ENDIF
    
    
    ;======================================================
    

    ; Locating the G0 stellar population parameters 

    testg0 = strupcase(strmid(key,0,2)) EQ 'G0' 

    ind = where(testg0,countindg0)

    
    ; retrieveing the defaut values from the txt database
    tstg0 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G0' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg0,ctdatg0)
    if ctdatg0 ne 0 then begin
         
        T_eff_MS_g0 = double(T_eff_MS(indat))
        R_star_MS_g0 = double(R_star_MS(indat))
        
    endif
    

    IF countindg0 NE 0 THEN BEGIN

        lumclassG0 = lumclass(ind)
        nlmG0 = n_elements(lumclassG0)
        indG0_1 = fltarr(nlmG0)
        indG0_2 = indG0_1
        indG0_3 = indG0_1
        indG0_4 = indG0_1
        countindG0_1 = indG0_1
        countindG0_2 = indG0_1
        countindG0_3 = indG0_1
        countindG0_4 = indG0_1
        FOR i=0L,nlmG0-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg0_1[i] =  where(testg0 and params EQ 1, countindg0_1x); index of radius of this stellar population in the val array
            countindg0_1[i] = countindg0_1x
            indg0_2[i] =  where(testg0 and params EQ 2, countindg0_2x); index of temperature of this stellar population in the val array
            countindg0_2[i] = countindg0_2x
            indg0_3[i] =  where(testg0 and params EQ 3, countindg0_3x); index of distance of this stellar population in the val array
            countindg0_3[i] = countindg0_3x
            indg0_4[i] =  where(testg0 and params EQ 4, countindg0_4x); index of the nstars of this stellar population in the val array
            countindg0_4[i] = countindg0_4x
        ENDFOR

    ENDIF
    
    ; Locating the G1 stellar population parameters

    testg1 = strupcase(strmid(key,0,2)) EQ 'G1'  

    ind = where(testg1,countindg1)

    
    ; retrieveing the defaut values from the txt database
    tstg1 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G1' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg1,ctdatg1)
    if ctdatg1 ne 0 then begin
         
        T_eff_MS_g1 = double(T_eff_MS(indat))
        R_star_MS_g1 = double(R_star_MS(indat))
        
    endif

    IF countindg1 NE 0 THEN BEGIN

        lumclassG1 = lumclass(ind)
        nlmG1 = n_elements(lumclassG1)
        indG1_1 = fltarr(nlmG1)
        indG1_2 = indG1_1
        indG1_3 = indG1_1
        indG1_4 = indG1_1    
        countindG1_1 = indG1_1
        countindG1_2 = indG1_1
        countindG1_3 = indG1_1
        countindG1_4 = indG1_1
        FOR i=0L,nlmG1-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg1_1[i] =  where(testg1 and params EQ 1, countindg1_1x); index of radius of this stellar population in the val array
            countindg1_1[i] = countindg1_1x
            indg1_2[i] =  where(testg1 and params EQ 2, countindg1_2x); index of temperature of this stellar population in the val array
            countindg1_2[i] = countindg1_2x
            indg1_3[i] =  where(testg1 and params EQ 3, countindg1_3x); index of distance of this stellar population in the val array
            countindg1_3[i] = countindg1_3x
            indg1_4[i] =  where(testg1 and params EQ 4, countindg1_4x); index of the nstars of this stellar population in the val array
            countindg1_4[i] = countindg1_4x
        ENDFOR

    ENDIF
    
    ; Locating the G2 stellar population parameters

    testg2 = strupcase(strmid(key,0,2)) EQ 'G2' 

    ind = where(testg2,countindg2) ;sun-like star

    ; retrieveing the defaut values from the txt database
    tstg2 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G2' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg2,ctdatg2)
    if ctdatg2 ne 0 then begin
         
        T_eff_MS_g2 = double(T_eff_MS(indat))
        R_star_MS_g2 = double(R_star_MS(indat))
        
    endif
    

    IF countindg2 NE 0 THEN BEGIN

        lumclassG2 = lumclass(ind)
        nlmG2 = n_elements(lumclassG2)
        indG2_1 = fltarr(nlmG2)
        indG2_2 = indG2_1
        indG2_3 = indG2_1
        indG2_4 = indG2_1
        countindG2_1 = indG2_1
        countindG2_2 = indG2_1
        countindG2_3 = indG2_1
        countindG2_4 = indG2_1
        FOR i=0L,nlmG2-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg2_1[i] =  where(testg2 and params EQ 1, countindg2_1x); index of radius of this stellar population in the val array
            countindg2_1[i] = countindg2_1x
            indg2_2[i] =  where(testg2 and params EQ 2, countindg2_2x); index of temperature of this stellar population in the val array
            countindg2_2[i] = countindg2_2x
            indg2_3[i] =  where(testg2 and params EQ 3, countindg2_3x); index of distance of this stellar population in the val array
            countindg2_3[i] = countindg2_3x
            indg2_4[i] =  where(testg2 and params EQ 4, countindg2_4x); index of the nstars of this stellar population in the val array
            countindg2_4[i] = countindg2_4x
        ENDFOR

    ENDIF
    
    ; Locating the G3 stellar population parameters

    testg3 = strupcase(strmid(key,0,2)) EQ 'G3' 

    ind = where(testg3,countindg3)

    ; retrieveing the defaut values from the txt database
    tstg3 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G3' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg3,ctdatg3)
    if ctdatg3 ne 0 then begin
         
        T_eff_MS_g3 = double(T_eff_MS(indat))
        R_star_MS_g3 = double(R_star_MS(indat))
        
    endif

    IF countindg3 NE 0 THEN BEGIN

        lumclassG3 = lumclass(ind)
        nlmG3 = n_elements(lumclassG3)
        indG3_1 = fltarr(nlmG3)
        indG3_2 = indG3_1
        indG3_3 = indG3_1
        indG3_4 = indG3_1   
        countindG3_1 = indG3_1
        countindG3_2 = indG3_1
        countindG3_3 = indG3_1
        countindG3_4 = indG3_1
        FOR i=0L,nlmG3-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg3_1[i] =  where(testg3 and params EQ 1, countindg3_1x); index of radius of this stellar population in the val array
            countindg3_1[i] = countindg3_1x
            indg3_2[i] =  where(testg3 and params EQ 2, countindg3_2x); index of temperature of this stellar population in the val array
            countindg3_2[i] = countindg3_2x
            indg3_3[i] =  where(testg3 and params EQ 3, countindg3_3x); index of distance of this stellar population in the val array
            countindg3_3[i] = countindg3_3x
            indg3_4[i] =  where(testg3 and params EQ 4, countindg3_4x); index of the nstars of this stellar population in the val array
            countindg3_4[i] = countindg3_4x
        ENDFOR

    ENDIF
    
    ; Locating the G4 stellar population parameters

    testg3 = strupcase(strmid(key,0,2)) EQ 'G4' 

    ind = where(testg3,countindg4)

    ; retrieveing the defaut values from the txt database
    tstg4 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G4' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg4,ctdatg4)
    if ctdatg4 ne 0 then begin
         
        T_eff_MS_g4 = double(T_eff_MS(indat))
        R_star_MS_g4 = double(R_star_MS(indat))
        
    endif

    IF countindg4 NE 0 THEN BEGIN

        lumclassG4 = lumclass(ind)
        nlmG4 = n_elements(lumclassG4)
        indG4_1 = fltarr(nlmG4)
        indG4_2 = indG4_1
        indG4_3 = indG4_1
        indG4_4 = indG4_1    
        countindG4_1 = indG4_1
        countindG4_2 = indG4_1
        countindG4_3 = indG4_1
        countindG4_4 = indG4_1
        FOR i=0L,nlmG4-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg4_1[i] =  where(testg3 and params EQ 1, countindg4_1x); index of radius of this stellar population in the val array
            countindg4_1[i] = countindg4_1x
            indg4_2[i] =  where(testg3 and params EQ 2, countindg4_2x); index of temperature of this stellar population in the val array
            countindg4_2[i] = countindg4_2x
            indg4_3[i] =  where(testg3 and params EQ 3, countindg4_3x); index of distance of this stellar population in the val array
            countindg4_3[i] = countindg4_3x
            indg4_4[i] =  where(testg3 and params EQ 4, countindg4_4x); index of the nstars of this stellar population in the val array
            countindg4_4[i] = countindg4_4x
        ENDFOR

    ENDIF
    
    ; Locating the G5 stellar population parameters

    testg5 = strupcase(strmid(key,0,2)) EQ 'G5' 

    ind = where(testg5,countindg5)

    ; retrieveing the defaut values from the txt database
    tstg5 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G5' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg5,ctdatg5)
    if ctdatg5 ne 0 then begin
         
        T_eff_MS_g5 = double(T_eff_MS(indat))
        R_star_MS_g5 = double(R_star_MS(indat))
        
    endif

    IF countindg5 NE 0 THEN BEGIN

        lumclassG5 = lumclass(ind)
        nlmG5 = n_elements(lumclassG5)
        indG5_1 = fltarr(nlmG5)
        indG5_2 = indG5_1
        indG5_3 = indG5_1
        indG5_4 = indG5_1
        countindG5_1 = indG5_1
        countindG5_2 = indG5_1
        countindG5_3 = indG5_1
        countindG5_4 = indG5_1
        FOR i=0L,nlmG5-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg5_1[i] =  where(testg5 and params EQ 1, countindg5_1x); index of radius of this stellar population in the val array
            countindg5_1[i] = countindg5_1x
            indg5_2[i] =  where(testg5 and params EQ 2, countindg5_2x); index of temperature of this stellar population in the val array
            countindg5_2[i] = countindg5_2x
            indg5_3[i] =  where(testg5 and params EQ 3, countindg5_3x); index of distance of this stellar population in the val array
            countindg5_3[i] = countindg5_3x
            indg5_4[i] =  where(testg5 and params EQ 4, countindg5_4x); index of the nstars of this stellar population in the val array
            countindg5_4[i] = countindg5_4x
       ENDFOR

    ENDIF
    
    ; Locating the G6 stellar population parameters

    testg6 = strupcase(strmid(key,0,2)) EQ 'G6' 
    ind = where(testg6,countindg6)
    ; retrieveing the defaut values from the txt database
    tstg6 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G6' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg6,ctdatg6)
    if ctdatg6 ne 0 then begin
         
        T_eff_MS_g6 = double(T_eff_MS(indat))
        R_star_MS_g6 = double(R_star_MS(indat))
        
    endif  

    IF countindg6 NE 0 THEN BEGIN

        lumclassG6 = lumclass(ind)
        nlmG6 = n_elements(lumclassG6) 
        indG6_1 = fltarr(nlmG6)
        indG6_2 = indG6_1
        indG6_3 = indG6_1
        indG6_4 = indG6_1 
        countindG6_1 = indG6_1
        countindG6_2 = indG6_1
        countindG6_3 = indG6_1
        countindG6_4 = indG6_1
        FOR i=0L,nlmG6-1 DO BEGIN     
            popnumber+=1
            countg+=1
            indg6_1[i] =  where(testg6 and params EQ 1, countindg6_1x); index of radius of this stellar population in the val array
            countindg6_1[i] = countindg6_1x
            indg6_2[i] =  where(testg6 and params EQ 2, countindg6_2x); index of temperature of this stellar population in the val array
            countindg6_2[i] = countindg6_2x
            indg6_3[i] =  where(testg6 and params EQ 3, countindg6_3x); index of distance of this stellar population in the val array
            countindg6_3[i] = countindg6_3x
            indg6_4[i] =  where(testg6 and params EQ 4, countindg6_4x); index of the nstars of this stellar population in the val array
            countindg6_4[i] = countindg6_4x
        ENDFOR

    ENDIF
    
    ; Locating the G7 stellar population parameters

    testg7 = strupcase(strmid(key,0,2)) EQ 'G7' 
    ind = where(testg7,countindg7)  
    ; retrieveing the defaut values from the txt database
    tstg7 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G7' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg7,ctdatg7)
    if ctdatg7 ne 0 then begin
         
        T_eff_MS_g7 = double(T_eff_MS(indat))
        R_star_MS_g7 = double(R_star_MS(indat))
        
    endif 

    IF countindg7 NE 0 THEN BEGIN

        lumclassG7 = lumclass(ind)
        nlmG7 = n_elements(lumclassG7)
        indG7_1 = fltarr(nlmG7)
        indG7_2 = indG7_1
        indG7_3 = indG7_1
        indG7_4 = indG7_1
        countindG7_1 = indG7_1
        countindG7_2 = indG7_1
        countindG7_3 = indG7_1
        countindG7_4 = indG7_1
        FOR i=0L,nlmG7-1 DO BEGIN 
            popnumber+=1
            countg+=1
            indg7_1[i] =  where(testg7 and params EQ 1, countindg7_1x); index of radius of this stellar population in the val array
            countindg7_1[i] = countindg7_1x
            indg7_2[i] =  where(testg7 and params EQ 2, countindg7_2x); index of temperature of this stellar population in the val array
            countindg7_2[i] = countindg7_2x
            indg7_3[i] =  where(testg7 and params EQ 3, countindg7_3x); index of distance of this stellar population in the val array
            countindg7_3[i] = countindg7_3x
            indg7_4[i] =  where(testg7 and params EQ 4, countindg7_4x); index of the nstars of this stellar population in the val array
            countindg7_4[i] = countindg7_4x
        ENDFOR

    ENDIF
    
    ; Locating the G8 stellar population parameters

    testg8 = strupcase(strmid(key,0,2)) EQ 'G8'     

    ind = where(testg8,countindg8)

    ; retrieveing the defaut values from the txt database
    tstg8 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G8' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg8,ctdatg8)
    if ctdatg8 ne 0 then begin
         
        T_eff_MS_g8 = double(T_eff_MS(indat))
        R_star_MS_g8 = double(R_star_MS(indat))
        
    endif

    IF countindg8 NE 0 THEN BEGIN

        lumclassG8 = lumclass(ind)
        nlmG8 = n_elements(lumclassG8)
        indG8_1 = fltarr(nlmG8)
        indG8_2 = indG8_1
        indG8_3 = indG8_1
        indG8_4 = indG8_1    
        countindG8_1 = indG8_1
        countindG8_2 = indG8_1
        countindG8_3 = indG8_1
        countindG8_4 = indG8_1
        FOR i=0L,nlmG8-1 DO BEGIN
            popnumber+=1
            countg+=1
            indg8_1[i] =  where(testg8 and params EQ 1, countindg8_1x); index of radius of this stellar population in the val array
            countindg8_1[i] = countindg8_1x
            indg8_2[i] =  where(testg8 and params EQ 2, countindg8_2x); index of temperature of this stellar population in the val array
            countindg8_2[i] = countindg8_2x
            indg8_3[i] =  where(testg8 and params EQ 3, countindg8_3x); index of distance of this stellar population in the val array
            countindg8_3[i] = countindg8_3x
            indg8_4[i] =  where(testg8 and params EQ 4, countindg8_4x); index of the nstars of this stellar population in the val array
            countindg8_4[i] = countindg8_4x
        ENDFOR

    ENDIF
    
    ; Locating the G9 stellar population parameters

    testg9 = strupcase(strmid(key,0,2)) EQ 'G9' 
    ind = where(testg9,countindg9)  
    ; retrieveing the defaut values from the txt database
    tstg9 = strtrim(strmid(SpecType_MS,0,2),2) EQ 'G9' and strtrim(strmid(SpecType_MS,2,1),2) NE '.'
    indat  = where(tstg9,ctdatg9)
    if ctdatg9 ne 0 then begin
         
        T_eff_MS_g9 = double(T_eff_MS(indat))
        R_star_MS_g9 = double(R_star_MS(indat))
        
    endif     

    IF countindg9 NE 0 THEN BEGIN

        lumclassG9 = lumclass(ind)
        nlmG9 = n_elements(lumclassG9)
        indG9_1 = fltarr(nlmG9)
        indG9_2 = indG9_1
        indG9_3 = indG9_1
        indG9_4 = indG9_1   
        countindG9_1 = indG9_1
        countindG9_2 = indG9_1
        countindG9_3 = indG9_1
        countindG9_4 = indG9_1
        FOR i=0L,nlmG9-1 DO BEGIN
            popnumber+=1   
            countg+=1
            indg9_1[i] =  where(testg9 and params EQ 1, countindg9_1x); index of radius of this stellar population in the val array
            countindg9_1[i] = countindg9_1x
            indg9_2[i] =  where(testg9 and params EQ 2, countindg9_2x); index of temperature of this stellar population in the val array
            countindg9_2[i] = countindg9_2x
            indg9_3[i] =  where(testg9 and params EQ 3, countindg9_3x); index of distance of this stellar population in the val array
            countindg9_3[i] = countindg9_3x
            indg9_4[i] =  where(testg9 and params EQ 4, countindg9_4x); index of the nstars of this stellar population in the val array
            countindg9_4[i] = countindg9_4x
        ENDFOR

    ENDIF
    

    comp_pop=replicate(one_pop,popnumber) ; Replication of the default and initialized stellar population structure to create the composite stellar population structure. All the tag values are by default set to te null value
    
    
    
    ;Filling the tags of the compsite stellar population structure using the indices defined above
    
    FOR i=0L,popnumber-1 DO BEGIN ; Looping over all the structure fields 
   
        IF counto NE 0 THEN BEGIN ; Filling the structure of the O STELLAR POPULATION(S)

            FOR k=0L,counto-1 DO BEGIN 

                IF countindo3 NE 0 THEN BEGIN

                    FOR l=0L,nlmO3-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'O3'+lumclasso3(l)+'_stellar_population'

                        IF countindo3_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo3_1[l]))(0)*rsun2cm ELSE BEGIN

;                             IF lumclasso3(l) EQ 'IA+' THEN comp_pop(k+i+l).radius = ;Hypergiants or extremely luminous supergiants
;                             IF lumclasso3(l) EQ 'IA' THEN comp_pop(k+i+l).radius =  ;Luminos supergiants
;                             IF lumclasso3(l) EQ 'IAB' THEN comp_pop(k+i+l).radius = ;Intermediate-size luminous supergiants
;                             IF lumclasso3(l) EQ 'IB' THEN comp_pop(k+i+l).radius =   ;Less luminous supergiants
;                             IF lumclasso3(l) EQ 'II' THEN comp_pop(k+i+l).radius =  ;Bright giants
;                             IF lumclasso3(l) EQ 'III' THEN comp_pop(k+i+l).radius = ;Normal giants
;                             IF lumclasso3(l) EQ 'IV' THEN comp_pop(k+i+l).radius =  ;Subgiants

                            IF lumclasso3(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o3*rsun2cm;15.0*rsun2cm ;(cm,cgs);Dwarfs: Main-sequence stars

;                             IF lumclasso3(l) EQ 'VI' THEN comp_pop(k+i+l).radius = ;Subdwarfs
;                             IF lumclasso3(l) EQ 'VII' THEN comp_pop(k+i+l).radius = ;White dwarfs   
                        ENDELSE
                        IF countindo3_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo3_2[l]))(0) ELSE BEGIN       
;                             IF lumclasso3(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso3(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso3(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso3(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso3(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso3(l) EQ 'III' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasso3(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso3(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o3;44.9e3 ;(K)

;                             IF lumclasso3(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso3(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =   
                        ENDELSE      
                        IF countindo3_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo3_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0 ; should be lower limited in the general procedure because this is the average distance between two stars
                        IF countindo3_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo3_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR
                    k+=nlmo3

                ENDIF
            
                IF countindo4 NE 0 THEN BEGIN

                    FOR l=0L,nlmO4-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'O4'+lumclasso4(l)+'_stellar_population'

                        IF countindo4_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo4_1[l]))(0)*rsun2cm ELSE BEGIN

;                             IF lumclasso4(l) EQ 'IA+' THEN comp_pop(k+i+l).radius = ;Hypergiants or extremely luminous supergiants
;                             IF lumclasso4(l) EQ 'IA' THEN comp_pop(k+i+l).radius =  ;Luminos supergiants
;                             IF lumclasso4(l) EQ 'IAB' THEN comp_pop(k+i+l).radius = ;Intermediate-size luminous supergiants
;                             IF lumclasso4(l) EQ 'IB' THEN comp_pop(k+i+l).radius    ;Less luminous supergiants
;                             IF lumclasso4(l) EQ 'II' THEN comp_pop(k+i+l).radius =  ;Bright giants
;                             IF lumclasso4(l) EQ 'III' THEN comp_pop(k+i+l).radius = ;Normal giants
;                             IF lumclasso4(l) EQ 'IV' THEN comp_pop(k+i+l).radius =  ;Subgiants

                            IF lumclasso4(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o4*rsun2cm;13.43*rsun2cm ;(cm,cgs);Dwarfs: Main-sequence stars

;                             IF lumclasso4(l) EQ 'VI' THEN comp_pop(k+i+l).radius = ;Subdwarfs
;                             IF lumclasso4(l) EQ 'VII' THEN comp_pop(k+i+l).radius = ;White dwarfs
                        ENDELSE
                        IF countindo4_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo4_2[l]))(0) ELSE BEGIN
;                             IF lumclasso4(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso4(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso4(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso4(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso4(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso4(l) EQ 'III' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasso4(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso4(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o4;42.9e3

;                             IF lumclasso4(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso4(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindo4_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo4_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindo4_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo4_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1  
                    ENDFOR 
                    k+=nlmo4 

                ENDIF
                
                
                IF countindo5 NE 0 THEN BEGIN

                    FOR l=0L,nlmo5-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'O5'+lumclasso5(l)+'_stellar_population'

                        IF countindo5_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo5_1[l]))(0)*rsun2cm ELSE BEGIN

;                             IF lumclasso5(l) EQ 'IA+' THEN comp_pop(k+i+l).radius = ;Hypergiants or extremely luminous supergiants
;                             IF lumclasso5(l) EQ 'IA' THEN comp_pop(k+i+l).radius =  ;Luminos supergiants
;                             IF lumclasso5(l) EQ 'IAB' THEN comp_pop(k+i+l).radius = ;Intermediate-size luminous supergiants
;                             IF lumclasso5(l) EQ 'IB' THEN comp_pop(k+i+l).radius    ;Less luminous supergiants
;                             IF lumclasso5(l) EQ 'II' THEN comp_pop(k+i+l).radius =  ;Bright giants
;                             IF lumclasso5(l) EQ 'III' THEN comp_pop(k+i+l).radius = ;Normal giants
;                             IF lumclasso5(l) EQ 'IV' THEN comp_pop(k+i+l).radius =  ;Subgiants

                            IF lumclasso5(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o5*rsun2cm;12*rsun2cm ;(cm,cgs);Dwarfs: Main-sequence stars

;                             IF lumclasso5(l) EQ 'VI' THEN comp_pop(k+i+l).radius = ;Subdwarfs
;                             IF lumclasso5(l) EQ 'VII' THEN comp_pop(k+i+l).radius = ;White dwarfs         
                        ENDELSE
                        IF countindo5_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo5_2[l]))(0) ELSE BEGIN
;                             IF lumclasso5(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso5(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso5(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso5(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso5(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso5(l) EQ 'III' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasso5(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso5(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o5;41.4e3

;                             IF lumclasso5(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso5(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                            IF countindo5_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo5_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                            IF countindo5_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo5_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                            ;K+=1
                    ENDFOR
                    k+=nlmo5         

                ENDIF
        
                
                
                IF countindo6 NE 0 THEN BEGIN

                    FOR l=0L,nlmo6-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'O6'+lumclasso6(l)+'_stellar_population'

                        IF countindo6_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo6_1[l]))(0)*rsun2cm ELSE BEGIN

;                             IF lumclasso6(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclasso6(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o6*rsun2cm;10.71*rsun2cm

;                             IF lumclasso6(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso6(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE 
                        IF countindo6_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo6_2[l]))(0) ELSE BEGIN
;                             IF lumclasso6(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso6(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o6;39.5e3

;                             IF lumclasso6(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso6(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindo6_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo6_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindo6_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo6_4[l]))(0) ELSE comp_pop(k+i+l).nstars = 1;stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1        
                    ENDFOR
                    k+=nlmo6

                ENDIF
        
                
                IF countindo7 NE 0 THEN BEGIN

                    FOR l=0L,nlmo7-1 DO BEGIN
                        comp_pop(k+l+i).popid = 'O7'+lumclass7(l)+'_stellar_population'
                        IF countindo7_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo7_1[l]))(0) ELSE BEGIN
;                             IF lumclasso7(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclasso7(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o7*rsun2cm;9.52*rsun2cm

;                             IF lumclasso7(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso7(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                            
                        ENDELSE
                        IF countindo7_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo7_2[l]))(0) ELSE BEGIN
;                             IF lumclasso7(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso7(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o7;37.1e3

;                             IF lumclasso7(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso7(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindo7_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo7_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindo7_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo7_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlmo7       

                ENDIF
                    
                
                IF countindo8 NE 0 THEN BEGIN

                    FOR l=0L,nlmo8-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'O8'+lumclasso8(l)+'_stellar_population'
                        IF countindo8_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo8_1[l]))(0) ELSE BEGIN
;                             IF lumclasso8(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclasso8(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o8*rsun2cm;8.5*rsun2cm

;                             IF lumclasso8(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso8(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindo8_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo8_2[l]))(0) ELSE BEGIN
;                             IF lumclasso8(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso8(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o8*rsun2cm;35.1e3

;                             IF lumclasso8(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso8(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindo8_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo8_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindo8_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo8_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1  
                    ENDFOR
                    k+=nlmo8       

                ENDIF
        
                
                IF countindo9 NE 0 THEN BEGIN

                    FOR l=0L,nlmo9-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'O9'+lumclasso9(l)+'_stellar_population'
                          
                        IF countindo9_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indo9_1[l]))(0) ELSE BEGIN  
;                             IF lumclasso9(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso9(l) EQ 'IA' THEN comp_pop(k+i+l).radius = 
                            IF lumclasso9(l) EQ 'IAB' THEN comp_pop(k+i+l).radius = 20.0*rsun2cm ;taken from Alnitak Aa's data. Even though its spec type is O9.5 (not O9)
;                             IF lumclasso9(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso9(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso9(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso9(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclasso9(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_o9*rsun2cm;7.51*rsun2cm

;                             IF lumclasso9(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclasso9(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindo9_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indo9_2[l]))(0) ELSE BEGIN
;                             IF lumclasso9(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso9(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
                            IF lumclasso9(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature = 29.5e3 ;taken from Alnitak Aa's data. Even though its spec type is O9.5 (not O9)
;                             IF lumclasso9(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso9(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso9(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso9(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasso9(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_o9*rsun2cm;33.3e3

;                             IF lumclasso9(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasso9(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                          
                        IF countindo9_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indo9_3[l]))(0) ELSE comp_pop(k+i+l).distance = 1.0E+00
                        IF countindo9_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indo9_4[l]))(0) ELSE comp_pop(k+i+l).nstars = 1;stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                           
                    ENDFOR
                    k+=nlmo9
                              

                ENDIF

                    
            ENDFOR

                  
            counto=0L 
    

        i+=k-1
        ENDIF

                    
    ;==============================================================================================
                
                        
        IF countb NE 0 THEN BEGIN ; Filling the structure of the B STELLAR POPULATION(S)
                    
            FOR k=0L,countb-1 DO BEGIN
                
                IF countindb0 NE 0 THEN BEGIN

                    FOR l=0L,nlmb0-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B0'+lumclassb0(l)+'_stellar_population'
                        IF countindb0_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb0_1[l]))(0) ELSE BEGIN
;                              IF lumclassb0(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                             IF lumclassb0(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b0*rsun2cm;7.16*rsun2cm

;                              IF lumclassb0(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                              IF lumclassb0(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb0_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb0_2[l]))(0) ELSE BEGIN
;                             IF lumclasb0(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb0(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b0;31.4e3

;                             IF lumclasb0(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb0(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindb0_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb0_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb0_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb0_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1         
                    ENDFOR
                    k+=nlmb0

                ENDIF
                
                
                
                IF countindb1 NE 0 THEN BEGIN

                    FOR l=0L,nlmb1-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B1'+lumclassb1(l)+'_stellar_population'
                        IF countindb1_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb1_1[l]))(0) ELSE BEGIN
;                             IF lumclassb1(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb1(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb1(l) EQ 'IAB' THEN comp_pop(k+i+l).radius = 
;                             IF lumclassb1(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb1(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb1(l) EQ 'III' THEN comp_pop(k+i+l).radius =
                            IF lumclassb1(l) EQ 'IV' THEN comp_pop(k+i+l).radius = 7.3*rsun2cm ;taken from Alnitak Ab's data.

                            IF lumclassb1(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b1*rsun2cm;5.71*rsun2cm

;                             IF lumclassb1(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb1(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb1_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb1_2[l]))(0) ELSE BEGIN
;                             IF lumclassb1(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassb1(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb1(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassb1(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassb1(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassb1(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
                            IF lumclassb1(l) EQ 'IV' THEN comp_pop(k+i+l).temperature = 29.0e3 ;taken from Alnitak Ab's data.

                            IF lumclassb1(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b1*rsun2cm;26.0e3

;                             IF lumclassb1(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassb1(l) EQ 'VII' THEN comp_pop(k+i+l).temperature = 
                        ENDELSE
                        IF countindb1_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb1_3[l]))(0) ELSE comp_pop(k+i+l).distance = 1.0E+00
                        IF countindb1_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb1_4[l]))(0) ELSE comp_pop(k+i+l).nstars = 1;stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmb1         

                ENDIF
                
                
                
                IF countindb2 NE 0 THEN BEGIN

                    FOR l=0L,nlmb2-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B2'+lumclassb2(l)+'_stellar_population'
                        IF countindb2_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb2_1[l]))(0) ELSE BEGIN
;                             IF lumclassb2(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb2(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b2*rsun2cm;4.06*rsun2cm

;                             IF lumclassb2(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb2(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb2_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb2_2[l]))(0) ELSE BEGIN
;                             IF lumclasb2(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb2(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b2;20.6e3 

;                             IF lumclasb2(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb2(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindb2_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb2_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb2_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb2_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmb2          

                ENDIF
                
                
                
                IF countindb3 NE 0 THEN BEGIN

                    FOR l=0L,nlmb3-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B3'+lumclassb3(l)+'_stellar_population'
                        IF countindb3_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb3_1[l]))(0) ELSE BEGIN
;                             IF lumclassb3(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb3(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b3*rsun2cm;3.61*rsun2cm

;                             IF lumclassb3(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb3(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb3_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb3_2[l]))(0) ELSE BEGIN
;                             IF lumclasb3(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb3(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b3;17.0e3

;                             IF lumclasb3(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb3(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindb3_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb3_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb3_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb3_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmb3          

                ENDIF
            
                IF countindb4 NE 0 THEN BEGIN

                    FOR l=0L,nlmb4-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B4'+lumclassb4(l)+'_stellar_population'
                        IF countindb4_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb4_1[l]))(0) ELSE BEGIN
;                             IF lumclassb4(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb4(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b4*rsun2cm;3.46*rsun2cm

;                             IF lumclassb4(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb4(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb4_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb4_2[l]))(0) ELSE BEGIN
;                             IF lumclasb4(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb4(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb4(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb4(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb4(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb4(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb4(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b4;16.4e3

;                             IF lumclasb4(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb4(l) EQ 'VII' THEN comp_pop(k+i+l).temperature = 
                        ENDELSE
                        IF countindb4_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb4_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb4_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb4_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmb4       

                ENDIF
                
                
                IF countindb5 NE 0 THEN BEGIN

                    FOR l=0L,nlmb5-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B5'+lumclassb5(l)+'_stellar_population'
                        IF countindb5_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb5_1[l]))(0) ELSE BEGIN
;                             IF lumclassb5(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb5(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b5*rsun2cm;3.36*rsun2cm

;                             IF lumclassb5(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb5(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb5_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb5_2[l]))(0) ELSE BEGIN
;                             IF lumclasb5(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb5(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b5;15.7e3 

;                             IF lumclasb5(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb5(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindb5_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb5_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb5_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb5_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmb5         

                ENDIF
        
                
                IF countindb6 NE 0 THEN BEGIN

                    FOR l=0L,nlmb6-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B6'+lumclassb6(l)+'_stellar_population'
                        IF countindb6_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb6_1[l]))(0) ELSE BEGIN
;                             IF lumclassb6(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb6(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b6*rsun2cm;3.27*rsun2cm

;                             IF lumclassb6(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb6(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb6_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb6_2[l]))(0) ELSE BEGIN
;                             IF lumclasb6(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasb6(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb6(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb6(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb6(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb6(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb6(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb6(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b6;14.5e3 

;                             IF lumclasb6(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb6(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindb6_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb6_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb6_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb6_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmb6        

                ENDIF
        
                
                IF countindb7 NE 0 THEN BEGIN

                    FOR l=0L,nlmb7-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B7'+lumclassb7(l)+'_stellar_population'
                        IF countindb7_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb7_1[l]))(0) ELSE BEGIN
;                             IF lumclassb7(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb7(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b7*rsun2cm;2.94*rsun2cm

;                             IF lumclassb7(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb7(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb7_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb7_2[l]))(0) ELSE BEGIN
;                             IF lumclasb7(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasb7(l) EQ 'IA' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasb7(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb7(l) EQ 'IB' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasb7(l) EQ 'II' THEN comp_pop(k+i+l).temperature =  
;                             IF lumclasb7(l) EQ 'III' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasb7(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb7(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b7;14.0e3   

;                             IF lumclasb7(l) EQ 'VI' THEN comp_pop(k+i+l).temperature = 
;                             IF lumclasb7(l) EQ 'VII' THEN comp_pop(k+i+l).temperature = 
                        ENDELSE
                        IF countindb7_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb7_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb7_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb7_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1  
                    ENDFOR
                    k+=nlmb7        

                ENDIF
                    
                
                IF countindb8 NE 0 THEN BEGIN

                    FOR l=0L,nlmb7-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'B8'+lumclassb8(l)+'_stellar_population'
                        IF countindb8_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb8_1[l]))(0) ELSE BEGIN
;                             IF lumclassb8(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb9(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb8(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb8(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb8(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb8(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb8(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassb8(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b8*rsun2cm;2.86*rsun2cm

;                             IF lumclassb8(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassb8(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindb8_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb8_2[l]))(0) ELSE BEGIN
;                             IF lumclasb8(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasb8(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b8;12.3e3 

;                             IF lumclasb8(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasb8(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindb8_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb8_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindb8_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb8_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1 
                    ENDFOR  
                    k+=nlmb8      

                ENDIF
        
                
                IF countindb9 NE 0 THEN BEGIN

                    FOR l=0L,nlmb9-1 DO BEGIN
                    comp_pop(k+i+l).popid = 'B9'+lumclassb9(l)+'_stellar_population'
                    IF countindb9_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indb9_1[l]))(0) ELSE BEGIN
;                         IF lumclassb9(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                        IF lumclassb9(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_b9*rsun2cm;2.49*rsun2cm

;                         IF lumclassb9(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                         IF lumclassb9(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                    ENDELSE
                    IF countindb9_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indb9_2[l]))(0) ELSE BEGIN
;                         IF lumclasb9(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                        IF lumclasb9(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_b9;10.7e3 

;                         IF lumclasb9(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                         IF lumclasb9(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                    ENDELSE
                    IF countindb9_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indb9_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                    IF countindb9_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indb9_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1 
                    ENDFOR
                    k+=nlmb9         

                ENDIF
                        
                    
            ENDFOR
                    
            countb=0. 
  
        i+=k-1
        ENDIF 

    ;==============================================================================================
                        
        IF counta NE 0 THEN BEGIN ; Filling the structure of the A STELLAR POPULATION(S)
                    
            FOR k=0L+i,counta-1+i DO BEGIN
                
                IF countinda0 NE 0 THEN BEGIN

                    FOR l=0L,nlma0-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A0'+lumclassa0(l)+'_stellar_population'
                        IF countinda0_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda0_1[l]))(0) ELSE BEGIN
;                             IF lumclassa0(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa0(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a0*rsun2cm;2.193*rsun2cm

;                             IF lumclassa0(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa0(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda0_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda0_2[l]))(0) ELSE BEGIN
;                             IF lumclasa0(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa0(l) EQ 'V' THEN comp_pop(k+i+l).temperature =T_eff_MS_a0; 9.7e3

;                             IF lumclasa0(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa0(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda0_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda0_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda0_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda0_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlma0        

                ENDIF
                
                
                
                IF countinda1 NE 0 THEN BEGIN

                    FOR l=0L,nlma1-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A1'+lumclassa1(l)+'_stellar_population'
                        IF countinda1_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda1_1[l]))(0) ELSE BEGIN
;                             IF lumclassa1(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa1(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a1*rsun2cm;2.136*rsun2cm

;                             IF lumclassa1(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa1(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda1_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda1_2[l]))(0) ELSE BEGIN
;                             IF lumclasa1(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa1(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a1;9.3e3

;                             IF lumclasa1(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa1(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda1_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda1_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda1_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda1_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                       ; K+=1 
                    ENDFOR 
                    k+=nlma1      

                ENDIF
                

                IF countinda2 NE 0 THEN BEGIN

                    FOR l=0L,nlma2-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A2'+lumclassa2(l)+'_stellar_population'
                        IF countinda2_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda2_1[l]))(0) ELSE BEGIN
;                             IF lumclassa2(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa2(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a2*rsun2cm;2.117*rsun2cm

;                             IF lumclassa2(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa2(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda2_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda2_2[l]))(0) ELSE BEGIN
;                             IF lumclasa2(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa2(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a2;8.8e3

;                             IF lumclasa2(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa2(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda2_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda2_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda2_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda2_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlma2        

                ENDIF
                
                
                
                IF countinda3 NE 0 THEN BEGIN

                    FOR l=0L,nlma3-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A3'+lumclassa3(l)+'_stellar_population'
                        IF countinda3_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda3_1[l]))(0) ELSE BEGIN
;                             IF lumclassa3(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa3(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a3*rsun2cm;1.861*rsun2cm

;                             IF lumclassa3(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa3(l) EQ 'VII' THEN comp_pop(k+i+l).radius = 
                        ENDELSE
                        IF countinda3_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda3_2[l]))(0) ELSE BEGIN
;                             IF lumclasa3(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa3(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a3;8.6e3

;                             IF lumclasa3(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa3(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda3_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda3_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda3_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda3_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlma3          

                ENDIF
            
                IF countinda4 NE 0 THEN BEGIN

                    FOR l=0L,nlma4-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A4'+lumclassa4(l)+'_stellar_population'
                        IF countinda4_1 NE 0 THEN comp_pop(k+i+l).radius = (val(inda4_1))(0) ELSE BEGIN
;                             IF lumclassa4(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa4(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a4*rsun2cm;1.794*rsun2cm

;                             IF lumclassa4(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa4(l) EQ 'VII' THEN comp_pop(k+i+l).radius = 
                        ENDELSE
                        IF countinda4_2 NE 0 THEN comp_pop(k+i+l).temperature = (val(inda4_2))(0) ELSE BEGIN
;                             IF lumclasa4(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa4(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a4;8.25e3

;                             IF lumclasa4(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa4(l) EQ 'VII' THEN comp_pop(k+i+l).temperature = 
                        ENDELSE
                        IF countinda4_3 NE 0 THEN comp_pop(k+i+l).distance = (val(inda4_3))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda4_4 NE 0 THEN comp_pop(k+i+l).nstars = (val(inda4_4))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlma4         

                ENDIF
                
                
                IF countinda5 NE 0 THEN BEGIN

                    FOR l=0L,nlma5-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A5'+lumclassa5(l)+'_stellar_population'
                        IF countinda5_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda5_1[l]))(0) ELSE BEGIN
;                             IF lumclassa5(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa5(l) EQ 'V' THEN omp_pop(k+i+l).radius = R_star_MS_a5*rsun2cm;1.785*rsun2cm

;                             IF lumclassa5(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa5(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda5_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda5_2[l]))(0) ELSE BEGIN
;                             IF lumclasa5(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa5(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a5;8.1e3

;                             IF lumclasa5(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa5(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda5_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda5_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda5_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda5_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1  
                    ENDFOR   
                    k+=nlma5     

                ENDIF
        
                
                IF countinda6 NE 0 THEN BEGIN

                    FOR l=0L,nlma6-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A6'+lumclassa6(l)+'_stellar_population'
                        IF countinda6_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda6_1[l]))(0) ELSE BEGIN
;                             IF lumclassa6(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa6(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a6*rsun2cm;1.775*rsun2cm

;                             IF lumclassa6(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa6(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda6_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda6_2[l]))(0) ELSE BEGIN
;                             IF lumclasa6(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa6(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a6;7.91e3 

;                             IF lumclasa6(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa6(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda6_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda6_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda6_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda6_5[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR 
                    k+=nlma6       

                ENDIF
        
                
                IF countinda7 NE 0 THEN BEGIN

                    FOR l=0L,nlma7-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A7'+lumclassa7(l)+'_stellar_population'
                        IF countinda7_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda7_1[l]))(0) ELSE BEGIN
;                             IF lumclassa7(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa7(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a7*rsun2cm;1.75*rsun2cm

;                             IF lumclassa7(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa7(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                         ENDELSE
                        IF countinda7_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda7_2[l]))(0) ELSE BEGIN
;                             IF lumclasa7(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa7(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa7(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa7(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa7(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa7(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa7(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a7;7.76e3

;                             IF lumclasa7(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa7(l) EQ 'VII' THEN comp_pop(k+i+l).temperature = 
                        ENDELSE
                        IF countinda7_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda7_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda7_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda7_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlma7       

                ENDIF
                    
                
                IF countinda8 NE 0 THEN BEGIN

                    FOR l=0L,nlma8-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A8'+lumclassa8(l)+'_stellar_population'
                        IF countinda8_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda8_1[l]))(0) ELSE BEGIN
;                             IF lumclassa8(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa8(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a8*rsun2cm;1.747*rsun2cm

;                             IF lumclassa8(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa8(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda8_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda8_2[l]))(0) ELSE BEGIN
;                             IF lumclasa8(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa8(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a8;7.590e3

;                             IF lumclasa8(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa8(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda8_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda8_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda8_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda8_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR 
                    k+=nlma8       

                ENDIF
        
                
                IF countinda9 NE 0 THEN BEGIN

                    FOR l=0L,nlma9-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'A9'+lumclassa9(l)+'_stellar_population'
                        IF countinda9_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(inda9_1[l]))(0) ELSE BEGIN
;                             IF lumclassa9(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassa9(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_a9*rsun2cm;1.747*rsun2cm

;                             IF lumclassa9(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassa9(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countinda9_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(inda9_2[l]))(0) ELSE begin
;                             IF lumclasa9(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclasa9(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_a9;7.4e3 

;                             IF lumclasa9(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclasa9(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countinda9_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(inda9_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countinda9_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(inda9_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlma9       

                ENDIF
                        
                        
            ENDFOR
                        
            counta=0. 
        i+=k-1
        ENDIF

                            
    ;==============================================================================================    
                        
                    
        IF countf NE 0 THEN BEGIN ; Filling the structure of the F STELLAR POPULATION(S)
                 
            FOR k=0L+i,countf-1+i DO BEGIN
                

                 IF countindf0 NE 0 THEN BEGIN
                    FOR l=0L,nlmaf0-1 DO BEGIN
                    comp_pop(k+i+l).popid = 'F0'+lumclassf0(l)+'_stellar_population'
                        IF countindf0_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf0_1[l]))(0) ELSE BEGIN
;                             IF lumclassf0(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf0(l) EQ 'V' THEN omp_pop(k+i+l).radius = R_star_MS_f0*rsun2cm;1.728*rsun2cm

;                             IF lumclassf0(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf0(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf0_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf0_2[l]))(0) ELSE BEGIN
;                             IF lumclassf0(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf0(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f0;7.22e3

;                             IF lumclassf0(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf0(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf0_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf0_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf0_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf0_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlmf0      

                ENDIF
                
                
                

                 IF countindf1 NE 0 THEN BEGIN
                    FOR l=0L,nlmaf1-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F1'+lumclassf1(l)+'_stellar_population'
                        IF countindf1_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf1_1[l]))(0) ELSE BEGIN
;                             IF lumclassf1(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf1(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f1*rsun2cm;1.679*rsun2cm

;                             IF lumclassf1(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf1(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf1_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf1_2[l]))(0) ELSE BEGIN
;                             IF lumclassf1(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf1(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f1;7.02e3

;                             IF lumclassf1(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf1(l) EQ 'VIII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf1_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf1_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf1_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf1_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1  
                    ENDFOR
                    k+=nlmf1        

                ENDIF
                
                
                
                IF countindf2 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf2-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F2'+lumclassf2(l)+'_stellar_population'
                        IF countindf2_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf2_1[l]))(0) ELSE BEGIN
;                             IF lumclassf2(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf2(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f2*rsun2cm;1.622*rsun2cm

;                             IF lumclassf2(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf2(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf2_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf2_2[l]))(0) ELSE BEGIN
;                             IF lumclassf2(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf2(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f2;6.820e3

;                             IF lumclassf2(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf2(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf2_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf2_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf2_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf2_4[l]))(0) ELSE comp_pop(k+i+l).nstars =  stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlmf2        

                ENDIF
                
                
                
                IF countindf3 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf3-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F3'+lumclassf3(l)+'_stellar_population'
                        IF countindf3_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf3_1[l]))(0) ELSE BEGIN
;                             IF lumclassf3(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf3(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f3*rsun2cm;1.578*rsun2cm

;                             IF lumclassf3(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf3(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf3_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf3_2[l]))(0) ELSE BEGIN
;                             IF lumclassf3(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf3(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f3;6.75e3

;                             IF lumclassf3(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf3(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf3_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf3_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf3_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf3_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR
                    k+=nlmf3         

                ENDIF
            
                IF countindf4 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf4-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F4'+lumclassf4(l)+'_stellar_population'
                        IF countindf4_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf4_1[l]))(0) ELSE BEGIN
;                             IF lumclassf4(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf4(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f4*rsun2cm;1.533*rsun2cm

;                             IF lumclassf4(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf4(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf4_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf4_2[l]))(0) ELSE BEGIN
;                             IF lumclassf4(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf4(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f4;6.67e3

;                             IF lumclassf4(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf4(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf4_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf4_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf4_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf4_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmf4          

                ENDIF
                
                
                IF countindf5 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf5-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F5'+lumclassf5(l)+'_stellar_population'
                        IF countindf5_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf5_1[l]))(0) ELSE BEGIN
;                             IF lumclassf5(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf5(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f5*rsun2cm;1.473*rsun2cm

;                             IF lumclassf5(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf5(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf5_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf5_2[l]))(0) ELSE BEGIN
;                             IF lumclassf5(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf5(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f5;6.55e3

;                             IF lumclassf5(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf5(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf5_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf5_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf5_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf5_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1
                    ENDFOR
                    k+=nlmf5          

                ENDIF
        
                
                IF countindf6 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf6-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F6'+lumclassf6(l)+'_stellar_population'
                        IF countindf6_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf6_1[l]))(0) ELSE BEGIN
;                             IF lumclassf6(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf6(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f6*rsun2cm;1.359*rsun2cm

;                             IF lumclassf6(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf6(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                         ENDELSE
                        IF countindf6_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf6_2[l]))(0) ELSE BEGIN
;                             IF lumclassf6(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf6(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f6;6.35e3

;                             IF lumclassf6(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf6(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf6_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf6_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf6_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf6_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmf6           

                ENDIF
        
                
                IF countindf7 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf7-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F7'+lumclassf7(l)+'_stellar_population'
                        IF countindf7_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf7_1[l]))(0) ELSE BEGIN
;                             IF lumclassf7(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf7(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f7*rsun2cm;1.324*rsun2cm

;                             IF lumclassf7(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf7(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf7_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf7_2[l]))(0) ELSE BEGIN
;                             IF lumclassf7(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf7(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f7;6.28e3

;                             IF lumclassf7(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf7(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindf7_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf7_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf7_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf7_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1 
                    ENDFOR
                    k+=nlmf7          

                ENDIF
                    
                
                IF countindf8 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf8-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F8'+lumclassf8(l)+'_stellar_population'
                        IF countindf8_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf8_1[l]))(0) ELSE BEGIN
;                             IF lumclassf8(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf8(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f8*rsun2cm;1.221*rsun2cm

;                             IF lumclassf8(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf8(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf8_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf8_2[l]))(0) ELSE BEGIN
;                             IF lumclassf8(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf8(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f8;6.18e3

;                             IF lumclassf8(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf8(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =   
                        ENDELSE
                        IF countindf8_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf8_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf8_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf8_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1
                    ENDFOR
                    k+=nlmf8           

                ENDIF
        
                
                IF countindf9 NE 0 THEN BEGIN

                    FOR l=0L,nlmaf9-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'F9'+lumclassf9(l)+'_stellar_population'
                        IF countindf9_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indf9_1[l]))(0) ELSE BEGIN
;                             IF lumclassf9(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassf9(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_f9*rsun2cm;1.167*rsun2cm

;                             IF lumclassf9(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassf9(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindf9_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indf9_2[l]))(0) ELSE BEGIN
;                             IF lumclassf9(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassf9(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_f9;6.05e3

;                             IF lumclassf9(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassf9(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =    
                        ENDELSE
                        IF countindf9_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indf9_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindf9_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indf9_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1 
                    ENDFOR
                    k+=nlmf9          

                ENDIF
                                    
                                        
            ENDFOR
                                                        
            countf=0.  
        i+=k-1
        ENDIF

                                                                    
    ;============================================================================================== 
                            
        IF countg NE 0 THEN BEGIN ; Filling the structure of the G STELLAR POPULATION(S)
                    
            FOR k=0L+i,countg-1+i DO BEGIN
                
                IF countindg0 NE 0 THEN BEGIN

                    FOR l=0L,nlmg0-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G0'+lumclassg0(l)+'_stellar_population'
                        IF countindg0_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg0_1[l]))(0) ELSE BEGIN
;                             IF lumclassg0(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg0(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g0*rsun2cm;1.1*rsun2cm

;                             IF lumclassg0(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg0(l) EQ 'VII' THEN comp_pop(k+i+l).radius =

                        ENDELSE
                        IF countindg0_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg0_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg0(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg0(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g0;5.93e3

;                             IF lumclassfg0(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg0(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg0_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg0_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg0_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg0_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR  
                    k+=nlmg0      

                ENDIF
                
                
                
                IF countindg1 NE 0 THEN BEGIN

                    FOR l=0L,nlmg1-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G1'+lumclassg1(l)+'_stellar_population'
                        IF countindg1_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg1_1[l]))(0) ELSE BEGIN
;                             IF lumclassg1(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg1(l) EQ 'V' THEN omp_pop(k+i+l).radius = R_star_MS_g1*rsun2cm;1.06*rsun2cm

;                             IF lumclassg1(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg1(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg1_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg1_2[l]))(0) ELSE begin
;                             IF lumclassfg1(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg1(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g1;5.86e3

;                             IF lumclassfg1(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg1(l) EQ 'VII' THEN comp_pop(k+i+l).temperature = 
                        ENDELSE
                        IF countindg1_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg1_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg1_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg1_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                    ;K+=1 
                    ENDFOR
                    k+=nlmg1

                ENDIF
                
                
                
                IF countindg2 NE 0 THEN BEGIN

                    FOR l=0L,nlmg2-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G2'+lumclassg2(l)+'_stellar_population'
                        IF countindg2_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg2_1[l]))(0) ELSE BEGIN
;                             IF lumclassg2(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg2(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g2*rsun2cm;1.012*rsun2cm

;                             IF lumclassg2(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg2(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg2_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg2_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg2(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg2(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g2;5.77e3

;                             IF lumclassfg2(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg2(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg2_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg2_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg2_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg2_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR
                    k+=nlmg2         

                ENDIF
                
                
                
                IF countindg3 NE 0 THEN BEGIN

                    FOR l=0L,nlmg3-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G3'+lumclassg3(l)+'_stellar_population'
                        IF countindg3_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg3_1[l]))(0) ELSE BEGIN
;                             IF lumclassg3(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg3(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g3*rsun2cm;1.002*rsun2cm

;                             IF lumclassg3(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg3(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg3_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg3_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg3(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg3(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g3;5.72e3

;                             IF lumclassfg3(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg3(l) EQ 'VII' THEN comp_pop(k+i+l).temperature 
                        ENDELSE
                        IF countindg3_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg3_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg3_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg3_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlmg3

                ENDIF
            
                IF countindg4 NE 0 THEN BEGIN

                    FOR l=0L,nlmg4-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G4'+lumclassg4(l)+'_stellar_population'
                        IF countindg4_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg4_1[l]))(0) ELSE BEGIN
;                             IF lumclassg4(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg4(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g4*rsun2cm;0.991*rsun2cm

;                             IF lumclassg4(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg4(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg4_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg4_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg4(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg4(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g4;5.68e3

;                             IF lumclassfg4(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg4(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg4_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg4_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg4_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg4_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1
                    ENDFOR
                    k+=nlmg4 

                ENDIF
                
                
                IF countindg5 NE 0 THEN BEGIN

                    FOR l=0L,nlmg5-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G5'+lumclassg5(l)+'_stellar_population'
                        IF countindg5_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg5_1[l]))(0) ELSE BEGIN
;                             IF lumclassg5(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg5(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g5*rsun2cm;0.977*rsun2cm

;                             IF lumclassg5(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg5(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg5_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg5_2[l]))(0) ELSE BEGIn
;                             IF lumclassfg5(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg5(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g5;5.66e3

;                             IF lumclassfg5(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg5(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg5_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg5_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg5_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg5_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlmg5       

                ENDIF
        
                
                IF countindg6 NE 0 THEN BEGIN

                    FOR l=0L,nlmg6-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G6'+lumclassg6(l)+'_stellar_population'
                        IF countindg6_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg6_1[l]))(0) ELSE BEGIN
;                             IF lumclassg6(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg6(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g6*rsun2cm;0.949*rsun2cm

;                             IF lumclassg6(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg6(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                         ENDELSE
                        IF countindg6_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg6_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg6(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg6(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g6;5.6e3

;                             IF lumclassfg6(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg6(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg6_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg6_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg6_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg6_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR
                    k+=nlmg6         

                ENDIF
        
                
                IF countindg7 NE 0 THEN BEGIN

                    FOR l=0L,nlmg7-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G7'+lumclassg7(l)+'_stellar_population'
                        IF countindg7_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg7_1[l]))(0) ELSE BEGIN
;                             IF lumclassg7(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg7(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g7*rsun2cm;0.927*rsun2cm

;                             IF lumclassg7(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg7(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg7_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg7_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg7(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg7(l) EQ 'V' THEN ccomp_pop(k+i+l).temperature = T_eff_MS_g7;5.55e3

;                             IF lumclassfg7(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg7(l) EQ 'VII' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg7_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg7_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg7_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg7_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR 
                    k+=nlmg7     

                ENDIF
                    
                
                IF countindg8 NE 0 THEN BEGIN

                    FOR l=0L,nlmg8-1 DO BEGIN
                        comp_pop(k+i+l).popid = 'G8'+lumclassg8(l)+'_stellar_population'
                        IF countindg8_1[l] NE 0 THEN comp_pop(k+i+l).radius = (val(indg8_1[l]))(0) ELSE BEGIN
;                             IF lumclassg8(l) EQ 'IA+' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'IA' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'IAB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'IB' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'II' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'III' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'IV' THEN comp_pop(k+i+l).radius =

                            IF lumclassg8(l) EQ 'V' THEN comp_pop(k+i+l).radius = R_star_MS_g8*rsun2cm;0.914*rsun2cm

;                             IF lumclassg8(l) EQ 'VI' THEN comp_pop(k+i+l).radius =
;                             IF lumclassg8(l) EQ 'VII' THEN comp_pop(k+i+l).radius =
                        ENDELSE
                        IF countindg8_2[l] NE 0 THEN comp_pop(k+i+l).temperature = (val(indg8_2[l]))(0) ELSE BEGIN
;                             IF lumclassfg8(l) EQ 'IA+' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'IA' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'IAB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'IB' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'II' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'III' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'IV' THEN comp_pop(k+i+l).temperature =

                            IF lumclassfg8(l) EQ 'V' THEN comp_pop(k+i+l).temperature = T_eff_MS_g8;5.48e3

;                             IF lumclassfg8(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
;                             IF lumclassfg8(l) EQ 'VI' THEN comp_pop(k+i+l).temperature =
                        ENDELSE
                        IF countindg8_3[l] NE 0 THEN comp_pop(k+i+l).distance = (val(indg8_3[l]))(0) ELSE comp_pop(k+i+l).distance = 10.0
                        IF countindg8_4[l] NE 0 THEN comp_pop(k+i+l).nstars = (val(indg8_4[l]))(0) ELSE comp_pop(k+i+l).nstars = stellar_density*(4.*!pi/3)*comp_pop(k+i+l).distance
                        ;K+=1 
                    ENDFOR
                    k+=nlmg8