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AIPS HELP file for SMODEL in 31DEC24

#### As of Fri Aug 9 7:10:22 2024

### HELP SECTION

SMODEL
Type: Adverb (REAL(7))
Use: This model specifies a point source model to use, usually instead
of a Clean components model. A non-zero flux density means this
model is to be used if appropriate. The elements of SMODEL are
SMODEL(1) = flux density (Jy)
SMODEL(2) = X offset in sky (arcsec)
SMODEL(3) = Y offset in sky (arcsec)
SMODEL(4) = Model type:
0 => point model
1 => elliptical Gaussian and
SMODEL(5) = major axis size (arcsec)
SMODEL(6) = minor axis size (arcsec)
SMODEL(7) = P. A. of major axis (degrees)
2 => uniform sphere and
SMODEL(5) = radius (arcsec)
3 => uniform sphere and
SMODEL(5) = radius (arcsec)
Null Value: 0
A null value of SMODEL(1) means no model is specified;
the useage of null values for other parameters depend on
the application.
Tasks:
BLCAL......Compute closure offset corrections.
BLCHN......Compute closure offset corrections on a channel-by-channel
basis.
BPASS......Computes spectral bandpass correction table.
CALIB......Determines antenna calibration: complex gain.
CPASS......Computes polynomial spectral bandpass correction table.
EVAUV......Subtracts & divides a model into UV data, does statistics
on results.
FRING......Fringe fit data to determine antenna calibration, delay,
rate.
KRING......Fringe fit data to determine antenna calibration, delay,
rate.
OOSUB......Subtracts/divides a model from/into a uv data base.
SCIMG......Full-featured imaging plus self-calibration loop with
editing.
SCMAP......Imaging plus self-calibration loop with editing.
UVADC......Fourier transforms and corrects a model and adds to uv
data.
UVCON......Generate sample UV coverage given a user defined array
layout.
UVSUB......Subtracts/divides a model from/into a uv data base.
Procedures:
OOCAL......Determines antenna complex gain with frequency-dependent
models.
OOFRING....Fringe fit data to determine calibration with spectral
index options.
VLBABPSS...Computes spectral bandpass correction table.

### EXPLAIN SECTION