FUNCTION dustem_compute_sed,p_dim,st,SED_spec,out_st=out_st,_extra=extra,wave0=wave0,help=help ;+ ; NAME: ; dustem_compute_sed ; PURPOSE: ; Computes an SED from a given Dustem trum ; 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 ; 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_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