dustem_fit_intensity_mbb_example.pro
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PRO dustem_fit_intensity_mbb_example,model=model $
,sed_file=sed_file $
,Nitermax=Nitermax $
,postscript=postscript $
,fits_save_and_restore=fits_save_and_restore $
,help=help $
,wait=wait $
,verbose=verbose
;+
; NAME:
; dustem_fit_intensity_mbb_example
;
; PURPOSE:
; This routine is an example of how to fit an observational SED
; (StokesI only) with DustEM and DustEMWrap.
;
; For this example, the code uses the SED in the file example_SED_1.xcat,
; which is distributed in the Data/EXAMPLE_OBSDATA/ directory
;
; In addition, this example uses the plugin dustem_plugin_mbbdy.pro to
; fit the FIR part of the spectrum using a modified black-body rather
; than a physical ISM dust model for the big grain population.
;
; The example SED has Stokes I photometric data points from
; IRAC, MIPS and IRAS. Examples illustrating running DustEMWrap to
; fit spectral data, polarisation data and extinction data
; are provided in other _example routines in the src/idl/
; directory. See the DustEMWrap User Guide for more information.
;
; CATEGORY:
; DustEMWrap, Distributed, High-Level, User Example
;
; CALLING SEQUENCE:
; dustem_fit_intensity_mbb_example[,model=][sed_file=][,postscript=][,Nitermax=][,fits_save_and_restore=][,/help,/wait,/verbose]
;
; 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 (default)
; '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)
; 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_1.xcat' is used.
; postscript = if set, final plot is saved as postscript in the
; current working directory
; 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
;
; 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:
; *** COMMENT AH --> is this really NONE? ****
;
; EXAMPLES
; dustem_fit_intensity_mbb_example
; dustem_fit_intensity_mbb_example,Nitermax=1,fits_save_and_restore='/tmp/mysavefile.fits'
; dustem_fit_intensity_mbb_example,model='DBP90'
;
; MODIFICATION HISTORY:
; Written by JPB Apr-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_intensity_mbb_example'
goto,the_end
END
IF keyword_set(model) THEN BEGIN
use_model=strupcase(model)
ENDIF ELSE BEGIN
use_model='MC10' ;Default is the DBP90 model
ENDELSE
use_polarization=0 ; initialize Dustemwrap in no polarization mode
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 (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.
;=== Examples are provided for some of the dust models.
;=== To try them, uncomment the model that you want to try and re-run
;=== AN EXAMPLE FOR DBP90
;=== Here we fit the
;=== intensity of the dust-heating radiation field as well as several plug-ins:
;=== (i) a modified black body (initial values correspond to a
; blackbody peaking in the far-infrared)
;=== The free parameters are all lower-bounded at zero.
;=== We invoke the MC10 dust model, and fit the abundances of the PAH components. The BG
;=== components are fixed to ~zero since we want to fit this part of the
;=== observed SED by a MBB.
;use_model='MC10' ; you should specify this when you run the routine!
pd = [ $
'(*!dustem_params).G0', $ ;G0
'(*!dustem_params).grains(0).mdust_o_mh',$ ;PAH0 mass fraction
'(*!dustem_params).grains(1).mdust_o_mh',$ ;PAH1 mass fraction
'dustem_plugin_mbbdy_1', $ ;Amplitude of mBB
'dustem_plugin_mbbdy_2', $ ;T of mBB
'dustem_plugin_mbbdy_3'] ;Emissivity index of mBB
iv = [1.8, 7.8e-4, 7.8e-4, 4.e-5, 22., 1.8]
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar)
llims=replicate(0.,Npar)
fpd = [ $
'(*!dustem_params).grains(2).mdust_o_mh',$ ;amCBEx
'(*!dustem_params).grains(3).mdust_o_mh',$ ;amCBEx
'(*!dustem_params).grains(4).mdust_o_mh'] ;aSilx
fiv = [1.e-12,1.e-12,1.e-12]
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
;!dustem_show_plot=1
;=== READ EXAMPLE SED DATA
dir=!dustem_wrap_soft_dir+'/Data/EXAMPLE_OBSDATA/'
file=dir+'example_SED_4.xcat'
IF keyword_set(sed_file) THEN file=sed_file
sed=read_xcat(file,/silent)
if keyword_set(wait) then begin
message,'Finished reading SED data: '+file,/info
wait,wait
end
;;=== ADJUST THE UNCERTAINTIES (FOR ILLUSTRATION)
ind=where(sed.sigmaII LT (0.2*sed.StokesI)^2,count)
IF count NE 0 THEN sed[ind].sigmaII=(0.2*sed[ind].StokesI)^2
;== SET THE OBSERVATIONAL STRUCTURE
;== sed is passed twice -- the first occurrence is the SED that you
;== wish to fit, the second occurrence is the SED that you wish to visualise.
dustem_set_data,sed,sed
;== SET INITIAL VALUES AND LIMITS OF THE PARAMETERS THAT WILL BE
;== ADJUSTED DURING THE FIT
;dustem_init_parinfo,pd,iv,up_limited=ulimed,lo_limited=llimed,up_limits=ulims,lo_limits=llims
;== INITIALIZE ANY PLUGINS
;dustem_init_plugins,pd,fpd
;== INITIALIZE ANY FIXED PARAMETERS FOR PLUGINS
;if Nfix gt 0 then dustem_init_fixed_params,fpd,fiv
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-16 ;fit tolerence
;=== INFORMATION TO MAKE THE PLOT
yr=[1.00e-4,1.00E2] ; y-axis limits
xr=[1.00E0,6.00e4] ; x-axis limits
tit='MBB FIT EXAMPLE' ; plot title
ytit=textoidl('I_\nu (MJy/sr) for N_H=10^{20} H/cm^2') ; y-axis title
xtit=textoidl('\lambda (\mum)') ; x-axis title
;Set show_plot to 0 to hide plot
;Commented or set to 1 is the same since !dustem_show_plot (existing sysvar) is initialized to 1 in dustem_init
;show_plot = 0
;=== RUN THE FIT
t1=systime(0,/sec)
res=dustem_mpfit_data(tol=tol,Nitermax=use_Nitermax,gtol=gtol $
,/xlog,/ylog,xr=xr,yr=yr,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
;=== MAKE THE FINAL PLOT
IF keyword_set(postscript) THEN BEGIN
dir_ps='./'
set_plot,'PS'
ps_file=dir_ps+postscript
device,filename=ps_file,/color
ENDIF
dustemwrap_plot,*(*!dustem_fit).CURRENT_PARAM_VALUES,dummy,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,title=tit+' (Final fit)'
IF keyword_set(postscript) THEN BEGIN
set_plot,'X'
device,/close
message,'Wrote '+ps_file,/info
ENDIF
if keyword_set(wait) then begin
message,'Made the plot of the final results',/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
dustem_read_fits_table,filename=fits_save_and_restore,dustem_spectra_st=dustem_spectra_st
;==== plot result taken from the saved fits table
res=*(*!dustem_fit).CURRENT_PARAM_VALUES
dustemwrap_plot,res,dustem_spectra_st,xr=xr,/xstyle,yr=yr,/ysty,/ylog,/xlog,title=tit+' (From Saved FITS file)'
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
end
ENDIF
message,'Finished dustem_fit_intensity_mbb_example',/info
stop
the_end:
END