dustem_compute_sed.pro
3.41 KB
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FUNCTION dustem_compute_sed,p_dim,st,$
SED_spec=SED_spec,out_st=out_st,$
wave0=wave0,$
_extra=extra,$
help=help
;+
; NAME:
; dustem_compute_sed
; PURPOSE:
; Computes an SED from a given Dustem model
; CATEGORY:
; Dustem
; CALLING SEQUENCE:
; sed=dustem_compute_sed(p_dim[,st][,sed_spec][out_st][,_extra=][,/help][wave0=])
; INPUTS:
; p_dim = parameter values (used only if st is not provided)
; OPTIONAL INPUT PARAMETERS:
; st = Dustem output structure, if provided, overrides p_dim
; wave0 = minimum wavelength for spectra (?)
; OUTPUTS:
; sed = computed SED for filters in !dustem_data
; sed_spec = computed spectrum
; OPTIONAL OUTPUT PARAMETERS:
; out_st = same as sed
; ACCEPTED KEY-WORDS:
; help = If set, print this help
; COMMON BLOCKS:
; None
; SIDE EFFECTS:
; None
; RESTRICTIONS:
; The dustem idl wrapper must be installed
; PROCEDURE:
; None
; EXAMPLES
;
; MODIFICATION HISTORY:
; Written by J.-Ph. Bernard
; Evolution details on the DustEMWrap gitlab.
; See http://dustemwrap.irap.omp.eu/ for FAQ and help.
;-
IF keyword_set(help) THEN BEGIN
doc_library,'dustem_compute_sed'
dustem_sed=0.
goto,the_end
ENDIF
IF not keyword_set(st) THEN BEGIN
dustem_activate_plugins,p_dim/(*(*!dustem_fit).param_init_values),st
;st=dustem_run(p_dim)
ENDIF
if not keyword_set(wave0) then wave0 = 0.
; Convert into MJy/sr/1d20
fact = 1.e4*(*!dustem_HCD)/(4.*!pi)/(3.e8/1.e-6/st.sed.wav)*1.e20/1.e7 ;this is correct despite the way it is presented (1.e4/1e.7*1e.20=1.e17 which is the factor to convert from ergs to Mega Janskys)
SED_spec = st.sed.em_tot * fact
;ADDING PLUGIN TO SPECTRUM----------------
scopes=tag_names((*!dustem_plugin))
IF scopes[0] NE 'NONE' THEN BEGIN
;IF ptr_valid(!dustem_plugin) THEN BEGIN
for i=0L,n_tags(*!dustem_plugin)-1 do begin
if total(strsplit((*(*!dustem_plugin).(i).scope),'+',/extract) eq 'ADD_SED') then SED_spec+=(*(*!dustem_plugin).(i).spec)[*,0]
endfor
ENDIF
;------------------------------------------
if not isarray(SED_spec) THEN stop
;COMPUTE THE MODEL SED
dustem_sed = (*(*!dustem_data).sed).values * 0.
IF !dustem_do_cc NE 0 AND !dustem_never_do_cc EQ 0 THEN BEGIN
message,'DOING color correction calculations',/info
ENDIF ELSE BEGIN
message,'SKIPPING color correction calculations: we take previous values of cc',/info
ENDELSE
ind_sed=where((*(*!dustem_data).sed).filt_names NE 'SPECTRUM' and (*(*!dustem_data).sed).wav gt wave0,count_sed)
IF count_sed NE 0 THEN BEGIN
filter_names=((*(*!dustem_data).sed).filt_names)[ind_sed]
ssed=dustem_cc(st.sed.wav,SED_spec,filter_names,cc=cc)
dustem_sed[ind_sed]=ssed
ENDIF ELSE BEGIN
print,"**** WARNING **** NO FILTER defined in DATA for COLOUR CORRECTION"
ENDELSE
;For spectrum data points, interpolate in log-log
;Linear interpolation leads to wrong values, in particular where few
;wavelengths points exist in the model (long wavelengths).
ind_spec=where((*(*!dustem_data).sed).filt_names EQ 'SPECTRUM',count_spec)
IF count_spec NE 0 THEN BEGIN
dustem_sed[ind_spec]=interpol(SED_spec,st.sed.wav,(((*(*!dustem_data).sed).wav)[ind_spec]))
;dustem_sed(ind_spec)=10^interpol(alog10(spec),alog10(st.sed.wav),alog10((((*!dustem_data.sed).wav)(ind_spec))))
ENDIF
out_st=st
;clean pointers
heap_gc
the_end:
;VG : error in cc IRAS1 when no PAH
; j=where(dustem_sed ne dustem_sed,count)
; if count gt 0 then dustem_sed[j]=0.
;stop
RETURN,dustem_sed
END