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[WEEDS\]MODSOURCE MODFILE ANTSIZE [/BACKGROUND TBG] [/OPACITY I]
Model the emission of a source at the local thermodynamic equilibrium
(LTE). The model paramaters (column density, kinetic temperature, source
size, line width and velocity offset for each species) are read from
MODFILE. The modeled antenna temperature is stored in the TB_MODEL memo-
ry. For convenience the current spectra is also stored in a memory, OBS,
so one can easily overplot the result of the model on the observed spec-
MODFILE the name of the file containing the parameters. The file
must have one line per species with at least six columns
1) The species name
2) The column density for this species in cm-2
3) The exitation temperature in K
4) The source size in arcsecs
5) The offset velocity from the source VLSR, in km/s
6) The line FWHM in km/s
One additional column may be used to select a different
origin for each species:
7) The origin of this species (e.g. JPL or CDMS). If emp-
ty, species with any origin are selected.
The following options may be used at the end of the line:
/ABSORPTION If this option is set, the component is as-
sumed to be a foreground layer. See Belloche et al. A&A
559, A47 (2013) for details.
/PARTFUNC Q Set the log10 of the partition function at
the excitation temperature to Q. If not set, the partition
function values (log-log interpolated/extrapolated at the
excitation temperature) from the selected database are
Lines that start with a "!" are treated as comments.
ANTSIZE the antenna size in meters
/BACKGROUND set the background temperature to TBG, in K. Default is
/OPACITY I store the opacity of the Ith component in the TAU_MODEL
memory. Components are numbered in the same order as in
MODFILE, starting from 1.
/VERBOSE prints partition function, lines frequencies, upper level
energies and degeneracies, Einstein coefficients and opac-
ity at the line center.