dustem_fit_spectro_example.pro
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PRO dustem_fit_spectro_example,model=model $
,sed_file=sed_file $
,postscript=postscript $
,Nitermax=Nitermax $
,fits_save=fits_save $
,ucfactor=ucfactor $
,wait=wait $
,noobj=noobj $
,help=help $
,verbose=verbose
;+
; NAME:
; dustem_fit_spectro_example
;
; PURPOSE:
; This routine is an example of how to fit spectrometer data in
; emission (StokesI only) with DustEM and DustEMWrap.
;
; See the DustEMWrap User Guide for more information.
;
; CATEGORY:
; DustEMWrap, Distributed, High-Level, User Example
;
; CALLING SEQUENCE:
; dustem_fit_spectro_example[,model=][sed_file=][ext_file=][postscript=][,Nitermax=][,fits_save=][,/help,/wait,/verbose,/noobj]
;
; INPUTS:
; None
;
; OPTIONAL INPUT PARAMETERS:
; None
;
; OUTPUTS:
; None
;
; OPTIONAL OUTPUT PARAMETERS:
; Plots, results structure in binary FITS table format
;
; ACCEPTED KEY-WORDS:
; model = specifies the interstellar dust mixture used by
; DustEM. See userguide or dustem_test_model_exists.pro
; for more details about available models in current release.
; sed_file = string naming the path to text file in .xcat format that
; describes the observational SED. If not set, the file
; 'Data/EXAMPLE_OBSDATA/example_SED_2.xcat' is used.
; Nitermax = maximum number of fit iterations. Default is 5.
; ucfactor = Multiplicative factor for uncertainties on
; spectrometer data. Default is 1.
; fits_save = if set, save the fit results in a binary
; FITS file.
; postscript = if set, final plot is saved as postscript file
; help = if set, print this help
; wait = if set, wait this many seconds between each step of
; the code (for illustration purposes)
; verbose = if set, subroutines will run in verbose mode
; noobj = if set, runs with no object graphics
;
; COMMON BLOCKS:
; None
;
; SIDE EFFECTS:
; None
;
; RESTRICTIONS:
; The DustEM fortran code must be installed
; The DustEMWrap IDL code must be installed
;
; PROCEDURES AND SUBROUTINES USED:
;
; EXAMPLES
; dustem_fit_spectro_example
; dustem_fit_spectro_example,Nitermax=10,fits_save='/tmp/mysavefile.fits'
; dustem_fit_spectro_example,model='DBP90'
;
; MODIFICATION HISTORY:
; Written by AH Oct 2022
; 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_fit_spectro_example'
goto,the_end
END
IF keyword_set(model) THEN BEGIN
use_model=strupcase(model)
ENDIF ELSE BEGIN
use_model='WD01_RV5P5B'
ENDELSE
exists=dustem_test_model_exists(use_model)
if exists eq 0 then $
message,'Unknown dust model'
use_polarization=0. ;default is no polarization in models
use_window=2 ; default graphics window number to use for plotting the results
use_verbose=0
if keyword_set(verbose) then use_verbose=1
use_ucfactor=1.
if keyword_set(ucfactor) then use_ucfactor=ucfactor
use_Nitermax=5 ; maximum number of iterations for the fit
IF keyword_set(Nitermax) THEN use_Nitermax=Nitermax
dustem_define_la_common
;=== Set the (model-dependent) parameters that you want to fit
;=== Refer to the DustEM and DustEMWrap userguides for an explanation
; of the different grain types
;=== Set the (model-dependent) parameters that you want to fit (pd),
;=== their initial values (iv)
;=== and whether they are bounded (ulimed,llimed,llims,ulims).
;=== Fixed parameters (fpd) and their values (fiv) are also set here.
;=== Refer to the DustEM and DustEMWrap User guides for an explanation
;=== of the physical meaning of dust model and plug-in parameters, and
;=== how to specify them.
;=== Example is provided for WD01_RV5P5B
;=== If you choose a different dust model, you will need to adjust the
;=== parameter information accordingly.
pd = [ '(*!dustem_params).G0', $ ; multiplicative factor of the radiation field
'(*!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
iv = [2., 5.4e-4, 5.4e-4, 1.8e-4, 1.65e-3, 7.e-3] ; starting guesses
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(1.e-15,Npar)
;=== Fixed parameters
fpd=[]
;=== Initial parameter values for fixed parameters
fiv=[]
if keyword_set(wait) then begin
message,'Finished setting dust model and plug-in parameters: '+use_model,/info
wait,wait
end
;== INITIALISE DUSTEM
dustem_init,model=use_model,polarization=use_polarization
!dustem_nocatch=1
!dustem_verbose=use_verbose
IF keyword_set(noobj) THEN !dustem_noobj=1
!EXCEPT=2 ; for debugging
;=== READ EXAMPLE EMISSION DATA TO FIT
dir=!dustem_wrap_soft_dir+'/Data/EXAMPLE_OBSDATA/'
file=dir+'example_SED_2.xcat'
if keyword_set(sed_file) then file=sed_file
sed=read_xcat(file,/silent)
;=== TWEAK THE UNCERTAINTIES ON THE SPECTROMETER DATA TO ADJUST THEIR
;=== RELATIVE WEIGHT IN THE FIT
fidx=where(sed.filter eq 'SPECTRUM',fct)
if fct gt 0 then sed[fidx].sigmaii = use_ucfactor*sed[fidx].sigmaii
;== SET THE OBSERVATIONAL STRUCTURE
dustem_set_data,m_fit=sed,m_show=sed
;== SET INITIAL VALUES AND LIMITS OF THE PARAMETERS FOR THE FIT
;== AND ACTIVATE ANY PLUGINS
dustem_init_params,use_model,pd,iv,fpd=fpd,fiv=fiv,ulimed=ulimed,llimed=llimed,ulims=ulims,llims=llims,polarization=use_polarization
if keyword_set(wait) then begin
message,'Finished initializing DustEMWrap, including plugins and fixed parameters',/info
wait,wait
end
;== INFORMATION TO RUN THE FIT
tol=1.e-10 ;fit tolerance
;=== INFORMATION TO MAKE THE PLOT
;=== _x/_extinction means extinction plots, _m/_emissions means emission plots
xr_m = [1.,5e5]
yr_m = [5e-8,1.00e6]
tit_m='FIT SPECTRO EXAMPLE' ; plot title
tit=tit_m
;=== RUN THE FIT
t1=systime(0,/sec)
res=dustem_mpfit_data(tol=tol,Nitermax=use_Nitermax,gtol=gtol $
,/xlog,/ylog,xr_m=xr_m,yr_m=yr_m,xr_x=xr_x,yr_x=yr_x,xtit=xtit,ytit=ytit,tit_m=tit_m $
,legend_xpos=legend_xpos,legend_ypos=legend_ypos $
,errors=errors,chi2=chi2,rchi2=rchi2,show_plot=show_plot)
t2=systime(0,/sec)
if keyword_set(wait) then begin
message,'Finished running DustEMWrap, using Niters: '+strtrim(string(use_Nitermax),2),/info
message,'Time taken [sec]: '+sigfig(t2-t1,2,/sci),/info
wait,wait
end
;=== MAKE THE FINAL PLOT
IF keyword_set(postscript) THEN BEGIN
; dir_ps='./'
mydevice=!d.name
set_plot,'PS'
; ps_file=dir_ps+postscript
ps_file=postscript
device,filename=ps_file,/color
ENDIF
;stop
IF !dustem_noobj THEN BEGIN
dustemwrap_plot_noobj,*(*!dustem_fit).CURRENT_PARAM_VALUES,st=dummy,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,title=tit+' (Final fit)'
ENDIF ELSE BEGIN
dustemwrap_plot,*(*!dustem_fit).CURRENT_PARAM_VALUES,st=dummy,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,title=tit+' (Final fit)'
ENDELSE
IF keyword_set(postscript) THEN BEGIN
device,/close
set_plot,mydevice
message,'Wrote '+ps_file,/info
ENDIF
IF keyword_set(fits_save) THEN BEGIN
message,'Writing out results structure: '+fits_save,/info
dustem_write_fits_table,filename=fits_save,help=help
;; Moved following to dustem_fitsio_example.pro
;; dustem_read_fits_table,filename=fits_save,dustem_st=dustem_spectra_st
;; res=*(*!dustem_fit).CURRENT_PARAM_VALUES
;; IF !dustem_noobj THEN BEGIN
;; dustemwrap_plot_noobj,res,dustem_spectra_st,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,tit_m=tit_m+' (From Saved FITS file)'
;; ENDIF ELSE BEGIN
;; dustemwrap_plot,res,dustem_spectra_st,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,tit_m=tit_m+' (From Saved FITS file)'
;; ENDELSE
IF keyword_set(wait) THEN BEGIN
message,'Saved the results as FITS in the file: '+fits_save,/info
wait,wait
ENDIF
ENDIF
the_end:
message,'Finished dustem_fit_spectro_example',/info
END