dustem_fit_spectro_example.pro
8.49 KB
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
PRO dustem_fit_spectro_example,model=model $
,sed_file=sed_file $
,Nitermax=Nitermax $
,fits_save_and_restore=fits_save_and_restore $
,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 an observational
; spectrometer data in emission (StokesI) 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=][,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)
; 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_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_spectro_example
; dustem_fit_spectro_example,Nitermax=10,fits_save_and_restore='/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
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_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, sed,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='Spectral Energy Distribution'
;=== 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
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
dustem_read_fits_table,filename=fits_save_and_restore,dustem_st=dustem_spectra_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_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_and_restore+', and made a plot using the data in this file',/info
wait,wait
ENDIF
ENDIF
message,'Finished dustem_fit_spectro_example',/info
the_end:
END