PRO dustem_fit_ext_example,model=model $ ,ext_file=ext_file $ ,Nitermax=Nitermax $ ,fits_save_and_restore=fits_save_and_restore $ ,wait=wait $ ,noobj=noobj $ ,help=help $ ,verbose=verbose ;+ ; NAME: ; dustem_fit_ext_example ; ; PURPOSE: ; This routine is an example of how to fit an observational extinction SED ; (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_ext_example[,model=][ext_file=][,Nitermax=][,fits_save_and_restore=][,/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 ; 'MC10' model from Compiegne et al 2010 ; 'DBP90' model from Desert et al 1990 ; 'DL01' model from Draine & Li 2001 ; 'WD01_RV5P5B' model from Weingartner & Draine 2002 with Rv=5.5 ; 'DL07' model from Draine & Li 2007 ; 'J13' model from Jones et al 2013, as updated in ; Koehler et al 2014 ; 'G17_ModelA' model A from Guillet et al (2018). Includes ; polarisation. See Tables 2 and 3 of that paper for details. ; 'G17_ModelB' model B from Guillet et al (2018) ; 'G17_ModelC' model C from Guillet et al (2018) ; 'G17_ModelD' model A from Guillet et al (2018) ; ext_file = string naming the path to text file in .xcat format that ; describes the observational extinction SED. If not set, the file ; 'Data/EXAMPLE_OBSDATA/Mathis90Fitz99_DISM_NH20.xcat' is used. ; Nitermax = maximum number of fit iterations. Default is 5. ; fits_save_and_restore = if set, save the fit results in a binary ; FITS file. The code then restore this file and plots ; the results using the saved results information. ; 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_ext_example ; dustem_fit_ext_example,Nitermax=1,fits_save_and_restore='/tmp/mysavefile.fits' ; dustem_fit_ext_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_ext_example' goto,the_end END IF keyword_set(model) THEN BEGIN use_model=strupcase(model) ENDIF ELSE BEGIN use_model='J13' ENDELSE known_mdls=['MC10','DBP90','DL01','WD01_RV5P5B','DL07','J13','G17_MODELA','G17_MODELB','G17_MODELC','G17_MODELD'] test_model = where(known_mdls eq use_model,ct) if ct eq 0 then begin message,'ISM dust model '+use_model+' unknown',/continue message,'Known models are MC10,DBP90,DL01,WD01_RV5P5B,DL07,J13,G17_MODELA,G17_MODELB,G17_MODELC,G17_MODELD',/continue stop end 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_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 J13 ;=== If you choose a different dust model, you will need to adjust the ;=== parameter information accordingly. pd = [ $ '(*!dustem_params).grains(0).mdust_o_mh'$ ;CM20 -- power law size distribution ,'(*!dustem_params).grains(1).mdust_o_mh'$ ;CM20 -- logN size distribution ,'(*!dustem_params).grains(2).mdust_o_mh' $ ;aPyM5 ,'(*!dustem_params).grains(3).mdust_o_mh' ] ;aOlM5 iv = [2.9e-3, 6.7e-4, 2.1e-3, 2.8e-3] ; starting guess for the fit 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 EXTINCTION DATA THAT WE WANT TO FIT dir=!dustem_wrap_soft_dir+'/Data/EXAMPLE_OBSDATA/' file=dir+'Mathis90Fitz99_DISM_NH20.xcat' IF keyword_set(ext_file) THEN file=ext_file ext=read_xcat(file,/silent) ;=== HERE WE SET THE DATA SO THAT THE COMPUTE_ FUNCTIONS BELOW HAVE ;=== THE NECESSARY FIELDS AND INFORMATION dustem_set_data,sed,sed,ext,ext ;== 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 ;=== INFORMATION TO MAKE THE PLOTS ;=== _x/_extinction means extinction plots, _m/_emissions means emission plots xr_x=[0.01,30] yr_x=[1.00E-10,10] tit='Dust Optical Depth' ;ytit=textoidl('I_\nu (MJy/sr) for N_H=10^{20} H/cm^2') ;xtit=textoidl('\lambda (\mum)') ;=== RUN THE FIT t1=systime(0,/sec) res=dustem_mpfit_data(tol=tol,Nitermax=use_Nitermax,gtol=gtol $ ,/xlog,/ylog,xr_x=xr_x,yr_x=yr_x,xtit=xtit,ytit=ytit,title=tit $ ,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 IF keyword_set(fits_save_and_restore) THEN BEGIN message,'Writing out results structure: '+fits_save_and_restore,/info dustem_write_fits_table,filename=fits_save_and_restore,help=help ;=== At this point, you could erase all dustem system variables, or exit idl... all the ;=== information needed to recover the results and remake the plots has been saved in the FITS table ;stop dustem_read_fits_table,filename=fits_save_and_restore,dustem_st=dustem_st ;==== plot result taken from the saved fits table res=*(*!dustem_fit).CURRENT_PARAM_VALUES IF !dustem_noobj THEN BEGIN dustemwrap_plot_noobj,res,dustem_st,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,title=tit+' (From Saved FITS file)' ENDIF ELSE BEGIN dustemwrap_plot,res,dustem_st,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,title=tit+' (From Saved FITS file)' ENDELSE IF keyword_set(wait) THEN BEGIN message,'Saved the results as FITS in the file: '+fits_save_and_restore+', and made a plot using the data in this file',/info wait,wait ENDIF ENDIF message,'Finished dustem_fit_ext_example',/info the_end: END