dustem_make_polarization_ext_example.pro
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PRO dustem_make_polarization_ext_example,model=model $
,wave=wave $
,next=next $
,outfile=outfile $
,help=help $
,verbose=verbose
;+
; NAME:
; dustem_make_polarization_ext_example
;
; PURPOSE:
; This is an example of how to generate an extinction curve using DustEMWrap.
; It is meant to be an example to follow when writing your own
; programs using DustEMWrap
;
; CATEGORY:
; DustEMWrap, Distributed, High-Level, User Example
;
; CALLING SEQUENCE:
; dustem_make_polarization_ext_example[,model=][,filters=][,/help]
;
; INPUTS:
; wave = wavelength range specified as [minwave,maxwave] in microns over which
; to construct the extinction curve. The resulting curve
; will be defined on the vector :
; wave_vector=10^(alog10(wave[0])+alog10(wave[1])*findgen(Next)/float(Next))
; default is [0.01,50]
; Next = number of measurements in the extinction curve. Default is 100.
;
; OPTIONAL INPUT PARAMETERS:
; None
;
; OUTPUTS:
; None
;
; OPTIONAL OUTPUT PARAMETERS:
; outfile = path+filename for .xcat output of the EXT
;
; ACCEPTED KEY-WORDS:
; model = if set, name of the DustEM dust model to use (default='G17_MODELD')
; help = If set print this help
; verbose = If set, subroutines will be more chatty
;
; COMMON BLOCKS:
; None
;
; SIDE EFFECTS:
; None
;
; RESTRICTIONS:
; The DustEM fortran code must be installed
; The DustEMWrap IDL code must be installed
;
; PROCEDURE:
; None
;
; EXAMPLES
; dustem_make_polarization_ext_example
; dustem_make_polarization_ext_example,model='G17_MODELC',outfile='my_polarized_ext.xcat'
;
; MODIFICATION HISTORY:
; Written by AH Nov-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_make_polarization_ext_example'
goto,the_end
ENDIF
dustem_define_la_common
IF keyword_set(model) THEN BEGIN
use_model=strupcase(model)
ENDIF ELSE BEGIN
use_model='G17_MODELD' ;Default is one of the Guillet et al (2017) models since they treat dust polarisation properties
ENDELSE
IF keyword_set(outfile) THEN BEGIN
use_outfile=outfile
ENDIF ELSE BEGIN
use_outfile='./polarization_ext.xcat'
ENDELSE
known_mdls=['MC10','DBP90','DL01','WD01_RV5P5B','DL07','J13','G17_MODELA','G17_MODELB','G17_MODELC','G17_MODELD']
pol_mdls=['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
test_model = where(pol_mdls eq use_model,ct)
if ct eq 0 then begin
message,'The only models with polarisation are G17_MODELA,G17_MODELB,G17_MODELC,G17_MODELD',/continue
stop
end
use_verbose=0
use_polarization=1
use_next=100 ; number of extinction measurements
use_wave=10^(alog10(0.01)+alog10(50)*findgen(use_next)/float(use_next)) ; wavelengths at which extinction is defined
if keyword_set(verbose) then use_verbose=1
if keyword_set(next) then use_next=next
if keyword_set(wave) then use_wave=10^(alog10(wave[0])+alog10(wave[1])*findgen(use_next)/float(use_next))
dustem_init,mode=use_model,polarization=use_polarization
!dustem_verbose=use_verbose
!dustem_nocatch=1
;=== initialize wavelengths for the EXTINCTION
ext=dustem_initialize_ext(use_next)
ext.instru='EXTINCTION'
ext.filter='SPECTRUM'
ext.wave=use_wave
;=== initialize IQU and associated errors to avoid problems when checking EXT in dustem_set_data.pro
ext[*].EXT_I=1.
ext.EXT_Q=ext.EXT_I/100.
ext.EXT_U=ext.EXT_I/100.
ext.SIGEXTII=ext.EXT_I/1000.
ext.SIGEXTQQ=ext.EXT_I/1000.
ext.SIGEXTUU=ext.EXT_I/1000.
ext.SIGEXTIQ=ext.EXT_I/1000.
ext.SIGEXTIU=ext.EXT_I/1000.
ext.SIGEXTQU=ext.EXT_I/1000.
;=== Set which model parameters to use for the EXT, this will depend
;=== on the selected dust model. For model parameters not specified
;=== here, the default Dustem fortran values will be used
pd = [ $
'(*!dustem_params).grains(0).mdust_o_mh', $ ;PAH0_MC10 mass fraction
'(*!dustem_params).grains(1).mdust_o_mh', $ ;amCBE_0.3333x mass fraction
'(*!dustem_params).grains(2).mdust_o_mh', $ ;aSil2001BE6pctG_0.4x mass fraction
'dustem_plugin_modify_dust_polx_2' $ ;Dust polarization angle in extinction
]
true_vals=[7.8000E-04,7.8000E-04,7.8000E-04, 52.]
Npar=n_elements(pd)
ulimed=replicate(0,Npar)
llimed=replicate(1,Npar) & llimed[3]=0
llims=replicate(0,Npar)
;== SET INITIAL VALUES AND LIMITS OF THE PARAMETERS FOR THE FIT
;== AND ACTIVATE ANY PLUGINS
;== FOR REASONS, WE NEED TO DO THIS DUSTEM_SET_DATA CALL
dustem_init_params,use_model,pd,true_vals,pol=use_polarization,fpd=fpd,fiv=fiv,ulimed=ulimed,llimed=llimed,ulims=ulims,llims=llims
;=== initialize the !dustem_data structure that will be used internally
;== note that m_fit and m_show do not exist -- this is deliberate
;== since we are not treating emission data
dustem_set_data,m_fit,m_show,ext,ext
;=== compute the extinction curve (I then QU) using the model and specified
;=== true_vals of parameters
dustem_iext=dustem_compute_ext(true_vals,st=ssti) ;sst is not set on purpose, for dustem_compute_ext to compute the ext using fortran code
toto=dustem_compute_stokext(true_vals,st=sstqu) ;this procedure also allows for the extraction of the spectra
dustem_qext = toto[0]
dustem_uext = toto[1]
ext.EXT_I=dustem_Iext
ext.EXT_Q=dustem_Qext
ext.EXT_U=dustem_Uext
;=== set uncertainties to I,Q,U
ext.SIGEXTII=abs(ext.EXT_I*0.000001)
ext.SIGEXTQQ=abs(ext.EXT_Q*0.000001)
ext.SIGEXTUU=abs(ext.EXT_U*0.000001)
;=== set covariances to 0.
ext.SIGEXTIQ=0.
ext.SIGEXTIU=0.
ext.SIGEXTQU=0.
;==== fill in dependent columns of the EXT.
ext=dustem_fill_ext_dependent_columns(ext)
;======== save the EXT to a file
write_xcat,ext,use_outfile
message,'Wrote '+use_outfile,/continue
;======== move the file to the Data/EXAMPLE_OBSDATA/ subdirectory
;filename_final=!dustem_wrap_soft_dir+'/Data/EXAMPLE_OBSDATA/my_example_EXT_###.xcat'
;str='cp '+use_outfile+' '+filename_final
;message,'Do '+str+' to make change permanent',/continue
the_end:
END