dustem_fit_sed_readme.pro
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PRO dustem_fit_sed_readme,postcript=postcript,mode=mode,help=help,png=png
;This Readme describes how to fit SEDs with dustem
;It runs on the SED stored into the file sample_SED.xcat
;in this directory. Remember that the goal here is not necessarily to
;obtain a good fit in the end, but to illustrate the method.
;The provided SED has only photometric data points from SPITZER
;IRAC and MIPS and IRAS. No spectrum data points.
;SPECTRUM data points can be included and the corresponding filter
;filed must read SPECTRUM. Note that its is note necessary
;to use the .xcat file format, and data SED can be provided
;manually, but the observation structure must have the structure shown below.
;Obviously, the dustem package must have been installed succesfully (see
;dustem_cvs_readme.txt for install instructions).
;+
; NAME:
; dustem_fit_sed_readme
; PURPOSE:
; This is an example of how to fit SEDs with the dustem wrapper.
; It is meant to be an example to follow when writing your own
; programs using the dustem IDL wrapper.
; It is not meant to reproduce the result in Compiegne et al 2010
; The SED used here is in sample_SED.xcat
; CATEGORY:
; Dustem
; CALLING SEQUENCE:
; dustem_fit_sed_readme,postcript=postcript,mode=mode,help=help
; INPUTS:
; None
; OPTIONAL INPUT PARAMETERS:
; None
; OUTPUTS:
; None
; OPTIONAL OUTPUT PARAMETERS:
; None
; ACCEPTED KEY-WORDS:
; mode = Selects one of the dust mixture used by dustem
; 'COMPIEGNE_ETAL2010' from Compiegne et al 2010 (default)
; 'DBP90' from Desert et al 1990
; 'DL01' from Draine & Li 2001
; 'DL07' from Draine & Li 2007
; postcript = if set plot is done in DUSTEM/Docs/Figures/Last_dustem_fit.ps
; 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:
; None
; EXAMPLES
; dustem_fit_sed_readme,mode='COMPIEGNE_ETAL2010'
; MODIFICATION HISTORY:
; Written by J.P. Bernard April 1st 2011
; see evolution details on the dustem cvs maintained at CESR
; Contact J.-Ph. Bernard (Jean-Philippe.Bernard@cesr.fr) in case of problems.
;-
IF keyword_set(help) THEN BEGIN
doc_library,'dustem_fit_sed_readme'
goto,the_end
ENDIF
IF keyword_set(mode) THEN BEGIN
use_mode=strupcase(mode)
ENDIF ELSE BEGIN
use_mode='COMPIEGNE_ETAL2010' ;Default is last dustem model
ENDELSE
IF keyword_set(png) THEN BEGIN
dir_png='/tmp/Dustem/Figures/'
force_mkdir,dir_png
ENDIF
;dbp=1
;=== initialise dustem
;dustem_init,/wrap
;dustem_init
dustem_init,mode=use_mode
!dustem_verbose=1
!dustem_show_plot=1
;=== Read sample SED
;;dir=getenv('DUSTEM_SOFT_DIR')+'/src/'
;dir=!dustem_wrap_soft_dir+'/Data/SEDs/'
;file=dir+'sample_SED.xcat'
;spec=read_xcat(file,/silent)
;=== Composite SED from Compiegne et al 2010, gathered by C. Bot
;dir=getenv('DUSTEM_SOFT_DIR')+'/src/dustem3.8_web/SEDs/'
dir=!dustem_wrap_soft_dir+'/Data/SEDs/'
file=dir+'Gal_composite_spectrum.xcat'
;file=dir+'Gal_composite_spectrum_wAKARI.xcat'
;stop
spec=read_xcat(file,/silent)
ind=where(spec.error EQ 0.,count)
IF count NE 0 THEN spec(ind).error=0.2*spec(ind).spec
ind=where(spec.instru EQ 'FIRAS',count)
IF count NE 0 THEN spec(ind).error=0.2*spec(ind).spec
;=== Draine Model SED for U=1. by C. Bot
;;dir=getenv('DUSTEM_SOFT_DIR')+'/src/dustem3.8_web/SEDs/'
;dir=!dustem_wrap_soft_dir+'/Data/SEDs/'
;file=dir+'SED_DraineModel_U1.0.xcat'
;spec=read_xcat(file,/silent)
;=== Fake SED made from Dustem outputs
;spec=dustem_compute_sed(p_dim,st=st,cont=cont,_extra=extra)
;=== Set which parameters you want to fit
;CASE getenv('DUSTEM_WHICH') OF
CASE !dustem_which OF
'WEB3p8':BEGIN
;=== This is to use Desert model
;=== must have done dustem_init,/DBP90
CASE use_mode OF
'DBP90':BEGIN
pd = [ $
'(*!dustem_params).G0', $ ;G0
'(*!dustem_params).grains(0).mdust_o_mh',$ ;PAH0 mass fraction
'(*!dustem_params).grains(1).mdust_o_mh',$ ;PAH1 mass fraction
'(*!dustem_params).grains(2).mdust_o_mh', $ ;amCBEx
'dustem_create_continuum_2'] ;Intensity of NIR continuum
iv = [1.0, 4.3e-4, 4.7e-4,6.4e-3,0.001]
; iv = [4.3e-4, 4.7e-4,6.4e-3,0.001]
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(0.,Npar)
;=== Fixed parameters
; fpd=['(*!dustem_params).G0'] ;Fixed parameter description
; fiv=[1.5]
; dustem_init_fixed_params,fpd,fiv
END
'DL01':BEGIN
pd = [ $
'(*!dustem_params).G0', $ ;G0
'(*!dustem_params).grains(0).mdust_o_mh',$ ;PAH0 mass fraction
'(*!dustem_params).grains(1).mdust_o_mh',$ ;PAH1 mass fraction
'(*!dustem_params).grains(2).mdust_o_mh', $ ;Gra
'(*!dustem_params).grains(3).mdust_o_mh', $ ;Gra
'(*!dustem_params).grains(4).mdust_o_mh', $ ;aSil
'dustem_create_continuum_2'] ;Intensity of NIR continuum
iv = [1.0,5.4e-4, 5.4e-4,1.8e-4,2.33e-3,8.27e-3,0.001]
; iv = [5.4e-4, 5.4e-4,1.8e-4,2.33e-3,8.27e-3,0.001]
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(0.,Npar)
;=== Fixed parameters
; fpd=['(*!dustem_params).G0'] ;Fixed parameter description
; fiv=[1.0]
; dustem_init_fixed_params,fpd,fiv
END
'DL07':BEGIN
pd = [ $
'(*!dustem_params).G0', $ ;G0
'(*!dustem_params).grains(0).mdust_o_mh',$ ;PAH0 mass fraction
'(*!dustem_params).grains(1).mdust_o_mh',$ ;PAH1 mass fraction
'(*!dustem_params).grains(2).mdust_o_mh', $ ;Gra
'(*!dustem_params).grains(3).mdust_o_mh', $ ;Gra
'(*!dustem_params).grains(4).mdust_o_mh', $ ;aSil
'dustem_create_continuum_2'] ;Intensity of NIR continuum
iv = [1.0,5.4e-4, 5.4e-4,1.8e-4,2.33e-3,8.27e-3,0.001]
; iv = [5.4e-4, 5.4e-4,1.8e-4,2.33e-3,8.27e-3,0.001]
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(0.,Npar)
;=== Fixed parameters
; fpd=['(*!dustem_params).G0'] ;Fixed parameter description
; fiv=[1.0]
; dustem_init_fixed_params,fpd,fiv
END
'COMPIEGNE_ETAL2010':BEGIN
; PUTTING G0 last DOES NOT WORK BECAUSE OF ORDER ISSUE
pd = [ $
'(*!dustem_params).G0', $ ;G0
'(*!dustem_params).grains(1).mdust_o_mh',$ ;PAH1 mass fraction
'(*!dustem_params).grains(0).mdust_o_mh',$ ;PAH0 mass fraction
'(*!dustem_params).grains(2).mdust_o_mh', $ ;amCBEx
'(*!dustem_params).grains(3).mdust_o_mh', $ ;amCBEx
'(*!dustem_params).grains(4).mdust_o_mh', $ ;aSil
'dustem_create_continuum_2'] ;Intensity of NIR continuum
iv = [1.0, 7.8e-4, 7.8e-4,1.65e-4,1.45e-3,7.8e-3,0.001]
; iv = [7.8e-4, 7.7e-4,1.65e-4,1.45e-3,7.8e-3,0.001]
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(0.,Npar)
;=== Fixed parameters
; fpd=['(*!dustem_params).G0'] ;Fixed parameter description
; fiv=[1.0]
; dustem_init_fixed_params,fpd,fiv
END
ENDCASE
END
ELSE: BEGIN
pd = ['(*!dustem_params).grains(0).propmass',$ ;PAH mass fraction
'(*!dustem_params).grains(1).propmass',$ ;VSG mass fraction
'(*!dustem_params).grains(2).propmass',$ ;BG mass fraction
'dustem_create_continuum_2', $ ;Intensity of NIR continuum
'dustem_create_isrf_1'] ;ISRF scaling factor
;=== set initial value of parameters you want to fit
iv = [7e-5, 8e-4,6.6e-3,0.001,4.]
;in this example, we enforce parameters to be >0 and Xisrf >3
;Caution, initial values must be within limits ...
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(0.,Npar)
END
ENDCASE
;=== SET THE OBSERVATION STRUCTURE
st=dustem_set_data(sed=spec)
;VG : dustem_set_data turned into a function to be used indifferently for sed, ext, polext
;dustem_set_data,spec
;defsysv, '!dustem_data', {sed:ptr_new()} ;Data to fit
;== SET THE FITTED PARAMETERS
dustem_init_parinfo,pd,iv,up_limited=ulimed,lo_limited=llimed,up_limits=ulims,lo_limits=llims
;==== below is to reset the defaults keywords for PAH which in newer version of the fortran include spin and mix, ...
;(*!dustem_params).grains[0].TYPE_KEYWORDS='logn'
;(*!dustem_params).grains[1].TYPE_KEYWORDS='logn'
(*!dustem_params).grains[0].TYPE_KEYWORDS='logn'
(*!dustem_params).grains[1].TYPE_KEYWORDS='logn'
;stop
;dustem_sort_params
;hprint,*(*!dustem_fit).param_descs
;hprint,*(*!dustem_fit).param_init_values
;hprint,*(*!dustem_fit).param_func
;=== RUN fit
tol=1.e-14
;tol=1.e-2
;Nitermax=20 ;maximum number of iteration. This is the criterium which will stop the fit procedure
Nitermax=2 ;maximum number of iteration. This is the criterium which will stop the fit procedure
loadct,13
!y.range=[1e-4,10] ;This is to ajust plot range from outside the routine
t1=systime(0,/sec)
res=dustem_mpfit_data(tol=tol,Nitermax=Nitermax,gtol=gtol,/xlog,/ylog)
;res=dustem_mpfit_sed(tol=tol,Nitermax=Nitermax) ;,func_name=func_name,cf_min=cf_min)
t2=systime(0,/sec)
;=== With FXD Model
;Final parameters : 0.00012425071 0.00022732277 0.0021897348 0.00047272697 4.4916225
;Iter 6 CHI-SQUARE = 76.345245 DOF = 6
;=== With MC Model
;Final parameters : 0.00012292305 0.00020672300 0.0020245400 0.00076911024 4.9751991
;Iter 6 CHI-SQUARE = 76.047516 DOF = 6
;=== With LV Model
;Final parameters : 0.00013302325 0.0010706767 0.0039392709 0.00074149811 4.7549752
;Iter 10 CHI-SQUARE = 90.478020 DOF = 6
;=== With LV Model using GRAIN_DBP.DAT
;Iter 7 CHI-SQUARE = 117.27229 DOF = 6
;Final parameters : 0.00011163016 0.00015163894 0.0017526653 0.00096639410 5.8391213
;stop
;=== SAVE FIT RESULTS
;file_out=getenv('DUSTEM_RES')+'DUSTEM_fit_example.sav'
file_out='/tmp/DUSTEM_fit_example.sav'
;dustem_save_sed_fit,file_out
dustem_save_system_variables,file_out
message,'Saved '+file_out,/continue
;stop
;======================================
;====You can exit IDL here and re-enter
;======================================
file='/tmp/DUSTEM_fit_example.sav'
dustem_restore_system_variables,file
;file=!dustem_res+'DUSTEM_fit_example.sav'
;dustem_restore_sed_fit,file
;=== Plot best fit
yr=[1e-4,10]
xr=[1,2000]
tit='DUSTEM Intensity SED fit Example (Saved)'
ytit=textoidl('I_\nu (MJy/sr) for N_H=10^{20} H/cm^2')
xtit=textoidl('\lambda (\mum)')
errors=(*(*!dustem_fit).current_param_errors)*(*(*!dustem_fit).param_init_values)
chi2=(*!dustem_fit).chi2
rchi2=(*!dustem_fit).rchi2
window,2
;=== RESTORE FIT RESULTS
;=== initialise dustem
;dustem_init,mode=use_mode
;file=getenv('DUSTEM_RES')+'DUSTEM_fit_example.sav'
;==== below is to reset the defaults keywords for PAH which in newer version of the fortran include spin and mix, ...
;(*!dustem_params).grains[0].TYPE_KEYWORDS='logn'
;(*!dustem_params).grains[1].TYPE_KEYWORDS='logn'
;=== recover best fit values
res=*(*!dustem_fit).current_param_values
chi2=(*!dustem_fit).chi2
rchi2=(*!dustem_fit).rchi2
errors=(*(*!dustem_fit).current_param_errors)*(*(*!dustem_fit).param_init_values)
;=== Plot best fit
loadct,13
IF keyword_set(postcript) THEN BEGIN
set_plot,'PS'
; ps_file=getenv('DUSTEM_SOFT_DIR')+'/Docs/Figures/'+'Last_dustem_fit.ps'
ps_file=!dustem_wrap_soft_dir+'/Docs/Figures/'+'Last_dustem_fit.ps'
device,filename=ps_file,/color
ENDIF
legend_xpos=2.
legend_ypos=1.
;dustem_sed_plot,(*!dustem_fit_params),ytit=ytit,xtit=xtit,title=tit,yr=yr,xr=xr,/ysty,/xsty,res=res,errors=errors,chi2=chi2,rchi2=rchi2
dustem_sed_plot,*(*!dustem_fit).current_param_values,ytit=ytit,xtit=xtit,title=tit,yr=yr,xr=xr,/ysty,/xsty,res=res,errors=errors,chi2=chi2,rchi2=rchi2,/xlog,/ylog,legend_xpos=legend_xpos,legend_ypos=legend_ypos
IF keyword_set(postcript) THEN BEGIN
device,/close
set_plot,'X'
message,'wrote '+ps_file,/info
ENDIF
IF keyword_set(png) THEN BEGIN
;file_png=!dustem_wrap_soft_dir+'/Docs/Figures/'+'Last_dustem_fit.png'
file_png=dir_png+'Last_dustem_fit_sed_readme.png'
write_png,file_png,tvrd(/true)
message,'Wrote '+file_png,/info
ENDIF
message,'dustem_mpfit_sed executed in '+strtrim(t2-t1,2)+' sec',/info
the_end:
END