pipeline.hifa.cli¶
Interferometry ALMA Tasks
Functions
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Derive and apply antenna position corrections for a list of MeasurementSets. |
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Performs temporal phase-up and derives bandpass calibration solutions. |
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Flag outlier visibilities in the bandpass calibrator data. |
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Compute optimal bandpass calibration solution intervals. |
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Derive SpW phase offsets from differential gain calibrator. |
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Export pipeline data products to the |
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Do metadata based flagging of a list of MeasurementSets. |
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Apply observatory-scientist flagging templates to science target data. |
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Locate and flag line regions in solar system flux calibrators. |
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Compute gaincal signal-to-noise ratios per spw. |
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Transfer the absolute flux scale from amplitude calibrator to secondary calibrators and science targets. |
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Flag outlier visibilities in the flux, diffgain, and phase calibrators and check source. |
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Select the optimal Briggs |
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Imports data into the interferometry pipeline. |
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Lock the reference antenna to a single antenna with |
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Perform per-session polarization calibration for ALMA. |
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Flag outlier visibilities in the polarization calibrator data. |
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Assess and optionally correct ALMA amplitude normalization errors caused by bright line emission. |
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Restore calibrated MeasurementSets from archived ASDMs and pipeline data products. |
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Select a single common reference antenna per session for polarization observations. |
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Compute phase calibration spw map and per spw phase offsets. |
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Flag target source outliers. |
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Determine temporal gains from calibrator observations. |
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Flag deviant system temperatures in the Tsys calibration table. |
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Flag astronomical line contamination in the system temperature (Tsys) calibration table. |
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Unlock reference antenna list. |
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Generate a gain table based on Water Vapor Radiometer (WVR) data. |
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Generate and apply a WVR phase correction table, flagging antennas with bad radiometers. |