PRO dustem_cc_print,filters,restart=restart,help=help

;+
; NAME:
;    dustem_cc_print
; PURPOSE:
;    Print out numerical values of color correction for a given spectrum in a given filter
;    This is a sanity checking routine.
;    Output should be compared to the color-correction tables published by different
;    instrument teams.

;    e.g. 1  MIPS HandBook, page 98

;    http://irsa.ipac.caltech.edu/data/SPITZER/docs/mips/mipsinstrumenthandbook/MIPS_Instrument_Handbook.pdf

;    http://irsa.ipac.caltech.edu/data/SPITZER/docs/mips/mipsinstrumenthandbook/51/
;    AND
;    e.g. 2  IRAS Explanatory Supplement, Table VI.C.6

;    https://irsa.ipac.caltech.edu/IRASdocs/exp.sup/ch6/tabsupC6.html  
; CATEGORY:

;    DustEMWrap, Distributed, Low-Level, User convenience

; CALLING SEQUENCE:
;    dustem_cc_print,filters[,restart=restart,help=help]
; INPUTS:
;    filter: names of filters for which color correction will be printed
; OPTIONAL INPUT PARAMETERS:
;    None
; OUTPUTS:
; OPTIONAL OUTPUT PARAMETERS:
; ACCEPTED KEY-WORDS:
;    help      = If set, print this help
;    restart   = If set, reinitialise DustEMWrap and use a new
;                wavelength vector for integration. 
; COMMON BLOCKS:
;    None
; SIDE EFFECTS:
;    None
; RESTRICTIONS:
;    The DustEM fortran code must be installed
;    The DustEMWrap IDL code must be installed
;    If restart is not set, this routine should be called after the
;    successful completion of a DustEMWrap run (i.e. without quitting the
;    IDL session) since it will use existing system variables 
; PROCEDURES AND SUBROUTINES USED:
;    *** COMMENT AH --> is this really NONE? ****
; EXAMPLES
;    dustem_print_cc,['MIRI1','MIRI6'],/restart
;    dustem_print_cc,['IRAS1','IRAC2']
; MODIFICATION HISTORY:
;    Written by JPB Apr-2011
;    Evolution details on the DustEMWrap gitlab.
;    See http://dustemwrap.irap.omp.eu/ for FAQ and help.  

;== Initialize DustemWrap if restart not requested
  if keyword_set(restart) then begin
     dustem_init

     Nwav=50000 & wavmin=0.1 & wavmax=500.

     wavs=findgen(Nwav)/(Nwav-1)*(wavmax-wavmin)+wavmin

     wavs=10^(alog10(wavmin)+alog10(wavmax)*(dindgen(Nwav+1)/Nwav))
     restart=0

  end else begin
     st=dustem_run()
     wavs=st.sed.wav
  end

;== Default filters to check
  if not keyword_set(filters) then begin
     message,'You must provide a list of filters',/info
     stop
  end

Nfilt=n_elements(filters)
wavref=dustem_filter2wav(filters)

;== Compute color corrections for power laws of frequency

pows=[2,1,0,-1,-2.]

Nv=n_elements(pows)
K=fltarr(Nv,Nfilt)

frmt_tit1='(A10,A10,A10,13F9.3)'
frmt1='(A10,A10,15F9.3)'

FOR i=0L,Nv-1 DO BEGIN

   spec=wavs^(-1.*pows[i])
   sed=dustem_cc(wavs,spec,filters,cc=cc,fluxconv=fluxconv,help=help)
   K[i,*]=cc

ENDFOR

print,'====== Power laws, spectral index between -3 and 3 ======'

print,'Filters','AltName','lambda0',pows,format=frmt_tit1

print,'========================================================='

FOR i=0L,Nfilt-1 DO print,filters[i],dustem_filter2name(filters[i]),wavref[i],K[*,i],format=frmt1

print,'========================================================='
print,'========================================================='
print,''

;== Compute color corrections for Black Bodies

Ts=[1.e4,5.e3,1.e3,500,200]

Nv=n_elements(Ts)
K=fltarr(Nv,Nfilt)

frmt_tit2='(A10,A10,A10,16I9)'

FOR i=0L,Nv-1 DO BEGIN
  spec=dustem_planck_function(Ts[i],wavs)
  sed=dustem_cc(wavs,spec,filters,cc=cc,fluxconv=fluxconv,help=help)
  K[i,*]=cc
ENDFOR

;== print results
print,'====== Blackbodies, temperatures between 20 and 10000K ======'

print,'Filters','AltName','lambda0',Ts,format=frmt_tit2

print,'============================================================='

FOR i=0L,Nfilt-1 DO print,filters[i],dustem_filter2name(filters[i]),wavref[i],K[*,i],format=frmt1

print,'============================================================='
print,'============================================================='

;stop

the_end:
END