pipeline.hifa.cli.hifa_timegaincal¶
-
pipeline.hifa.cli.
hifa_timegaincal
= <pipeline.hifa.cli.hifa_timegaincal._hifa_timegaincal object>¶ hifa_timegaincal —- Determine temporal gains from calibrator observations
The time-dependent complex gains for each antenna/spwid are determined from the raw data (DATA column) divided by the model (MODEL column), for the specified fields. The gains are computed independently for each specified spectral window. One gain solution is computed for the calibrator source targets and one for the science targets.
Previous calibrations are applied on the fly.
The complex gains are derived from the data column (raw data) divided by the model column (usually set with hif_setjy). The gains are obtained for the specified solution intervals, spw combination and field combination. One gain solution is computed for the science targets and one for the calibrator targets.
Good candidate reference antennas can be determined using the hif_refant task.
Previous calibrations that have been stored in the pipeline context are applied on the fly. Users can interact with these calibrations via the hif_export_calstate and hif_import_calstate tasks.
Output
results – If pipeline mode is ‘getinputs’ then None is returned. Otherwise the results object for the pipeline task is returned.
——— parameter descriptions ———————————————
- vis The list of input MeasurementSets. Defaults to the list of
MeasurementSets specified in the pipeline context.
example: vis=[‘M82A.ms’, ‘M82B.ms’]
- calamptable The list of output diagnostic calibration amplitude tables for
the calibration targets. Defaults to the standard pipeline naming convention.
example: calamptable=[‘M82.gacal’, ‘M82B.gacal’]
- offsetstable The list of output diagnostic phase offset tables for the
calibration targets. Defaults to the standard pipeline naming convention.
example: offsetstable=[‘M82.offsets.gacal’, ‘M82B.offsets.gacal’]
- calphasetable The list of output calibration phase tables for the
calibration targets. Defaults to the standard pipeline naming convention.
example: calphasetable=[‘M82.gcal’, ‘M82B.gcal’]
- targetphasetable The list of output phase calibration tables for the science
targets. Defaults to the standard pipeline naming convention.
example: targetphasetable=[‘M82.gcal’, ‘M82B.gcal’]
- amptable The list of output calibration amplitude tables for the
calibration and science targets. Defaults to the standard pipeline naming convention.
example: amptable=[‘M82.gcal’, ‘M82B.gcal’]
- field The list of field names or field ids for which gain solutions are to
be computed. Defaults to all fields with the standard intent.
example: field=’3C279’, field=’3C279, M82’
- intent A string containing a comma delimited list of intents against which
the selected fields are matched. Defaults to the equivalent of ‘AMPLITUDE,PHASE,BANDPASS’.
example: intent=’’, intent=’PHASE’
- spw The list of spectral windows and channels for which gain solutions are
computed. Defaults to all science spectral windows.
example: spw=’3C279’, spw=’3C279, M82’
antenna calsolint Time solution interval in CASA syntax for calibrator source
solutions.
example: calsolint=’inf’, calsolint=’int’, calsolint=’100sec’
- targetsolint Time solution interval in CASA syntax for target source
solutions.
example: targetsolint=’inf’, targetsolint=’int’, targetsolint=’100sec’
- combine Data axes to combine for solving. Options are ‘’, ‘scan’, ‘spw’,
‘field’ or any comma-separated combination.
default: ‘’ example: combine=’’
- refant Reference antenna name(s) in priority order. Defaults to most recent
values set in the pipeline context. If no reference antenna is defined in the pipeline context use the CASA defaults.
example: refant=’DV01’, refant=’DV05,DV07’
- refantmode Controls how the refant is applied. Currently available
choices are ‘flex’, ‘strict’, and the default value of ‘’. Setting to ‘’ allows the pipeline to select the appropriate mode based on the state of the reference antenna list.
Examples: refantmode=’strict’, refantmode=’’
solnorm Normalise the gain solutions. minblperant Minimum number of baselines required per antenna for each solve.
Antennas with fewer baselines are excluded from solutions.
example: minblperant=2
calminsnr Solutions below this SNR are rejected for calibrator solutions. targetminsnr Solutions below this SNR are rejected for science target
solutions.
- smodel Point source Stokes parameters for source model (experimental)
Defaults to using standard MODEL_DATA column data.
example: smodel=[1,0,0,0] - (I=1, unpolarized)
- pipelinemode The pipeline operating mode. In ‘automatic’ mode the pipeline
determines the values of all context defined pipeline inputs automatically. In interactive mode the user can set the pipeline context defined parameters manually. In ‘getinputs’ mode the user can check the settings of all pipeline parameters without running the task.
- dryrun Run the commands (True) or generate the commands to be run but do not
execute (False).
- acceptresults Add the results of the task to the pipeline context (True) or
reject them (False).
——— examples ———————————————————–
1. Compute standard per scan gain solutions that will be used to calibrate the target:
hifa_timegaincal()