CASA Contributed Task: makeschedule: Difference between revisions
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Download task files: Download task files: [[File:Task_select_sequence.py]], [[File:Findsources.xml]] | Download task files: Download task files: [[File:Task_select_sequence.py]], [[File:Findsources.xml]] | ||
Task to create complete schedules for JVLA observations that can be imported as a scan lists into the OPT, | |||
including initial setup, observations of flux and banpass calibrators, pointing scans, and phase calibrators. | |||
The task can run either on a pre-defined 'pointing_file' in SCT format, or it can generate a mosaic either in | |||
equatorial (J2000.0) or galactic coordinates centered at a specific 'position'. | |||
If many sources at different positions in the sky are observed, the program will pick the closest phase | |||
calibrator from 'phase_cals' and group sources related to each phase calibrator together. The task will then | |||
schedule the groups in the order of the list of phase calibrators given in 'phase_cals'. Phase calibrators with | |||
no associated targets will be ignored. | |||
The task will try to optimize the sequence of pointings, by always selecting the closest remaining target source | |||
for optimization = 'simple'. The 'complex' optimization can reduce settling times and gain a few seconds on source, | |||
but it runs much slower (in particular for large mosaics with a few hundred pointings). This is only recomended for | |||
mosacis with very short time per pointing (e.g. 12 seconds). | |||
Output files are: | |||
pointings.pst -- File with pointing positions in SCT format to be read into the OPT. | |||
scan_list_xxLST.opt -- Scan list to be imported to the OPT (import scans) for the specified LST start time. | |||
regions.reg -- Region file for ds9 |
Revision as of 18:09, 15 May 2012
Download task files: Download task files: File:Task select sequence.py, File:Findsources.xml
Task to create complete schedules for JVLA observations that can be imported as a scan lists into the OPT,
including initial setup, observations of flux and banpass calibrators, pointing scans, and phase calibrators.
The task can run either on a pre-defined 'pointing_file' in SCT format, or it can generate a mosaic either in
equatorial (J2000.0) or galactic coordinates centered at a specific 'position'.
If many sources at different positions in the sky are observed, the program will pick the closest phase calibrator from 'phase_cals' and group sources related to each phase calibrator together. The task will then schedule the groups in the order of the list of phase calibrators given in 'phase_cals'. Phase calibrators with no associated targets will be ignored.
The task will try to optimize the sequence of pointings, by always selecting the closest remaining target source for optimization = 'simple'. The 'complex' optimization can reduce settling times and gain a few seconds on source, but it runs much slower (in particular for large mosaics with a few hundred pointings). This is only recomended for mosacis with very short time per pointing (e.g. 12 seconds).
Output files are:
pointings.pst -- File with pointing positions in SCT format to be read into the OPT. scan_list_xxLST.opt -- Scan list to be imported to the OPT (import scans) for the specified LST start time. regions.reg -- Region file for ds9