AIPS HELP file for INLIST in 31DEC24
As of Sat Oct 5 15:20:44 2024
HELP SECTION
INLIST
Type: Adverb (String*48)
Use: To specify the name of a disk file outside the usual AIPS
catalog system to be used as input for an AIPS verb or task.
The file is a FITS- or other binary-format file representing
either image or UV data in binary form.
Format: The name is usually given by specifying a logical device plus
directory, followed by a colon, followed by the actual file
name. In Unix, logicals are environment variables. The
logical name must be set up before entering the AIPS program
and is usually in upper case. Thus, for example:
percent setenv MYAREA ~joeuser
for the C shell, and
$ myarea=$HOME; export MYAREA
for bourne, korn, and bash shells. Then in AIPS,
INLIST = 'MYAREA:FITS.DAT'
Note that the Unix-standard $ ahead of the logical is omitted.
AIPS-standard logicals like FITS (often AIPS/FITS) are available
also. Other forms are now acceptable as well:
INLIST = 'FITS.DAT
will find the file in the $FITS directory (when reading or
writing FITS disk files) or in the directory local when you
started AIPS. A full path name may also be given
INLIST = '/home/primate2/egreisen/AIPS/N6503.fits
if it fits in 48 characters. Note that the trailing quote mark
is left off and this is the last command on the input line so
that the case is preserved.
Null value: ' '
Taken to mean no subsidiary file. This can be an error.
Tasks:
BOXES........Adds Clean boxes to BOXFILE around sources from a
list; INLIST gives the source list
FACES........Makes images of catalog sources for initial
calibration; INLIST gives the source list
IMMOD........Adds images of model objects to an image.
INLIST contains a list of source models to be added.
MODAB........Makes simple absorption/emission spectral-line image
in I/V. INLIST contains a list of spectral lines
to put in the images.
MODIM........Adds images of model objects to image cubes in IQU
polarization. INLIST contains a list of sources
(fluxes, RM parameters, spatial parameters).
MODSP........Adds images of model objects to image cubes in I/V
polarization. INLIST contains a list of sources
(fluxes, spatial parameters, spectral parameters)
MTARS........Compute model inputs to TARS. INLIST contains a
list of sources (Q, U, RM parameters)
PANEL........Convert HOLOG output to panel adjustment table.
INLIST specifies VLA or VLBA or focal length and
panel structure.
SETFC........Makes a BOXFILE for input to IMAGR; INLIST gives the
list of possibly interfering sources
SPMOD........Modify UV database by adding a model with spectral
lines. INLIST gives a list of components (fluxes,
spatial and spectral parameters) to be added.
UVFIT........Fits source models to uv data. INLIST is an optional
list of initial guesses for the component parameters.
UVGIT........Fits source models to uv data. INLIST is an optional
list of initial guesses for the component parameters.
UVMOD........Modify UV database by adding a model incl spectral
index. INLIST is an optional list of components
to be included, required is want > 4.
EXPLAIN SECTION