AIPS HELP file for VLBAMCAL in 31DEC25
As of Wed Mar 26 8:10:36 2025
VLBAMCAL: Procedure to merge redundant calibration data
INPUTS
INNAME Input file name
INCLASS Input file class
INSEQ Input file sequence number
INDISK Disk number for input file
BADDISK List of disks not to be used
for scratch files.
VLBAMCAL is defined in the VLBAUTIL run file.
HELP SECTION
VLBAMCAL
Type: Procedure
Use: VLBAMCAL is a procedure that removes redundant calibration records
from data from the VLBA correlator. Note that VLBALOAD and
VLBAFIX will do this automatically.
Type RUN VLBAUTIL to make the VLBAMCAL procedure available.
INNAME.....The name of the file to be corrected. Wildcard characters
are allowed.
INCLASS....The class of the file to be corrected. Wildcard characters
are allowed.
INSEQ......The sequence number of the file to be corrected.
0 => highest number matching INNAME, INSEQ, and INDISK.
INDISK.....The disk drive number of the file to be corrected.
0 => any disk.
BADDISK....A list of disk numbers that are not to be used for scratch
files.
EXPLAIN SECTION
VLBAMCAL: Procedure to merge redundant calibration data.
Documentor: Chris Flatters, Amy Mioduszewski
Related Programs: FITLD, VLBALOAD, VLBAUTIL, MERGECAL, VLBAFIX
Note that VLBALOAD and VLBAFIX run VLBAMCAL.
WHEN TO USE VLBAMCAL
Use VLBAMCAL to get rid of redundant records in calibration tables.
These result from the duplication of certain calibration data across
FITS file boundaries in VLBA export tapes and can cause AIPS programs
(notably APCAL) to fail.
You should run VLBAMCAL after you have finished loading the data from
tape but before you either change the polarization structure of the data
with FXPOL, load any calibration data for non-VLBA telescopes, or apply
the calibration data.
VLBAMCAL is intended for all levels of VLBA users and can be used in
place of the older MERGECAL procedure.
WHAT TO DO NEXT
After you have removed the redundant calibration records, you should
search for possible subarraying conditions with VLBASUBS. If you are
confident that there are no subarrays in your data and you have dual
polarization data then you will need to fix the polarization labelling
with VLBAFPOL or FXPOL.