- corrected 04-Apr-2024
PIPELINE COLLECT and the subsequent
PIPELINE APPLY
could fail if some spectral windows had different flags than others, leading to different
time stamps or antenna numbers. Solved by using a fallback solution in which the closest
(in frequency) self-calibration solution is used instead of the (non available) delay
self-calibration. This loses some precision, though.
-
Corrected 10-Mar-2024
fits-to-uvt.ima was no longer working with option
/WEIGHT due to obsolete task uv_casa (probably since early 2019 !...).
Also
UV_REWEIGHT /FILE was not working correctly.
-
Corrected 08-Mar-2024
UV_PREVIEW was occasionally incorrectly identifying
line emission, leaving no line-free channel. This lead the
PIPELINE to crash, as no
Continuum image could be created. Algorithm has been improved.
- 07-Mar-2024 CASA keeps producing incomplete UVFITS files. Allow the
READ command to recover what is possible in such cases. Although visibilities are
in general complete (except perhaps the last one), these incomplete files will most likely miss
the absolute coordinates information that must be supplied manually by
UV_FIELDS.
-
Corrected 05-Mar-2024,
Discovered 6-Feb-2024
PIPELINE /MODE SURVEY was not working
properly when strong lines were present in spectral window.
- 05-Mar-2024 Implement
STATISTIC /FILE option
-
Corrected 22-Feb-2024
KEPLER MASK was using wrong velocity sign
-
Corrected 22-Feb-2024
MASK 3-D masks were incorrectly aligned
in Frequency: it ought to be in Velocity.
- 17-Feb-2024 Implement
WRITE CCT /APPEND
- 14-Feb-2024 Protect
CATALOG from empty (or out of range) catalogs.
- 11-Feb-2024 Allow use of
SHOW NOISE Buffer
- 06-Feb-2024 Improve polarization scripts to handle multiple spectral windows at once
-
Corrected 15-Jan-2024
UV_FILTER /FILE was crashing, due to
incorrect handling of the Flags.
UV_FILTER/ZERO now transmit
these flags correctly.
