Commit bfd73a3c08b13de5fd6b2b99bb601913a8764f66

Authored by Annie Hughes
1 parent b71e81d2
Exists in master

modified doc-help text

Showing 1 changed file with 25 additions and 17 deletions   Show diff stats
src/idl/dustem_show_fortran.pro
1   -PRO dustem_show_fortran, model=model, data_dir=data_dir,dustem_dir=dustem_dir,nh=nh, fsed=fsed, sw=sw, inst=inst, smdat=smdat, com=com, wref=wref, bbpar=bbpar, wext=wext, $
2   - xr=xr, yr=yr, tit=tit, CMB=cmb, COSMO=COSMO, DATA=data, SHOW=show, wn=wn, HARD=hard
  1 +PRO dustem_show_fortran, model=model $
  2 + , data_dir=data_dir $
  3 + , dustem_dir=dustem_dir $
  4 + , nh=nh, fsed=fsed, sw=sw $
  5 + , inst=inst, smdat=smdat, com=com $
  6 + , wref=wref, bbpar=bbpar, wext=wext $
  7 + , xr=xr, yr=yr, tit=tit $
  8 + , CMB=cmb, COSMO=COSMO, DATA=data, SHOW=show $
  9 + , wn=wn, HARD=hard
3 10  
4 11 ;+
5 12 ; NAME:
6 13 ; dustem_show_fortran
7 14 ; PURPOSE:
8   -; shows differents results of the DUSTEM fortran calculations,
9   -; overlaid on fiducial diffuse ISM dust observables
  15 +; shows various outputs of the DUSTEM fortran calculations,
  16 +; overlaid on an example observation of diffuse ISM dust
10 17 ; CATEGORY:
11 18 ; DustEM, Distributed, User-Example
12 19 ; CALLING SEQUENCE:
13   -; dustem_show_results
  20 +; dustem_show_fortran
14 21 ; INPUTS:
15   -; DATA_DIR : path to directory containing fiducial observational
16   -; SED files. Defaults to Data/EXAMPLE_OBSDATA/ subdirectory.
  22 +; DATA_DIR : path to directory containing observational
  23 +; SED files. Defaults to Data/EXAMPLE_OBSDATA/ subdirectory.
17 24 ; DUSTEM_DIR : path to directory containing DustEM data files. Default
18 25 ; is the !dustem_dat directory (which is defined in
19 26 ; a user's idl_startup file)
... ... @@ -77,26 +84,27 @@ PRO dustem_show_fortran, model=model, data_dir=data_dir,dustem_dir=dustem_dir,nh
77 84 ; EXAMPLES
78 85 ;; print,' Examples:'
79 86 ;; print,' path=''/Users/lverstra/DUSTEM_LOCAL/dustem4.0/'''
80   - ;; print,' to show SED only: show_dustem,path'
81   - ;; print,' SED+UV-extinction: show_dustem,path,show=''extuv'' '
82   - ;; print,' SED+IR extinction+size dist.: show_dustem,path,show=[''extir'',''sdist''] '
83   - ;; print,' ps files with default names: show_dustem,path,show=[''extir'',''alb''],/hard '
84   - ;; print,' ps files with given names: show_dustem,path,show=[''extir'',''sdist''],hard=[''f1.ps'',''f2.ps''] '
85   - ;; print,' no plot : show_dustem,path,show=0'
86   - ;; print,' to get band fluxes in structure SM: show_dustem,path,smdat=sm'
  87 + ;; print,' to show SED only: dustem_show_fortran,path'
  88 + ;; print,' SED+UV-extinction: dustem_show_fortran,path,show=''extuv'' '
  89 + ;; print,' SED+IR extinction+size dist.: dustem_show_fortran,path,show=[''extir'',''sdist''] '
  90 + ;; print,' ps files with default names: dustem_show_fortran,path,show=[''extir'',''alb''],/hard '
  91 + ;; print,' ps files with given names: dustem_show_fortran,path,show=[''extir'',''sdist''],hard=[''f1.ps'',''f2.ps''] '
  92 + ;; print,' no plot : dustem_show_fortran,path,show=0'
  93 + ;; print,' to get band fluxes in structure SM: dustem_show_fortran,path,smdat=sm'
87 94 ;; print,' see structure SM (overall): help,/str,sm'
88 95 ;; print,' see structure SM model field: help,/str,sm.m_emis'
89 96 ;; print,' see structure SM inst field: help,/str,sm.i_dirbe'
90 97 ;; print,' see structure SM inst flux field: help,/str,sm.i_dirbe.flx'
91 98 ;; print,' array(i,j+1) i:index of inst band, j:index of grain type (ntype+1 is total SED) '
92   - ;; print,' to select or add instrument field(s): show_dustem,path,smdat=sm,inst=[''spire''] (on existing SM to add instrumentx) '
  99 + ;; print,' to select or add instrument field(s): dustem_show_fortran,path,smdat=sm,inst=[''spire''] (on existing SM to add instrumentx) '
93 100 ; MODIFICATION HISTORY:
  101 +; Inherited from DustEM fortran repo, July 2022.
94 102 ; Written by L Verstraete and M Compiegne, Spring 2010
95 103 ; Modified by LV : change to cgs, add band fluxes in SMDAT, 2011
96 104 ; Modified by LV & V Guillet : add polarization part, 2017
97 105 ; Further evolution details on the DustEMWrap gitlab.
98 106 ; See http://dustemwrap.irap.omp.eu/ for FAQ and help.
99   -
  107 +;
100 108  
101 109 if keyword_set(help) then begin
102 110 doc_library,'dustem_show_fortran'
... ... @@ -186,7 +194,7 @@ if keyword_set(data_dir) then data_path = data_dir
186 194 ;
187 195 ; get the SED data
188 196 ;
189   -; New FarIR-mm SED from FBoulanger
  197 +; FarIR-mm SED from FBoulanger
190 198 RESTORE, data_path+'/EXAMPLE_OBSDATA/filters_ref_wave.xdr'
191 199 fact_em = 0.77 ; to account for 20% of H to be in ionized form + 3% H2
192 200 to_sed_20 = 1d-17 * (1d20/1.82d18) ; MJy/sr->erg/s/cm2/sr and normalization to NH = 10^20 H/cm2
... ...