Functions | |
def | wvrgcal |
def task_wvrgcal.wvrgcal | ( | vis = None , |
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caltable = None , |
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toffset = None , |
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segsource = None , |
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sourceflag = None , |
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tie = None , |
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nsol = None , |
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disperse = None , |
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wvrflag = None , |
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statfield = None , |
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statsource = None , |
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smooth = None , |
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scale = None , |
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reversespw = None , |
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cont = None |
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) |
Generate a gain table based on Water Vapour Radiometer data vis -- Name of input visibility file default: none; example: vis='ngc5921.ms' caltable -- Name of output gain calibration table default: none; example: caltable='ngc5921.wvr' toffset -- Time offset (sec) between interferometric and WVR data default: -1 (ALMA default) segsource -- Do a new coefficient calculation for each source default: True tie -- Prioritise tieing the phase of these sources as well as possible (requires segsource=True) default: [] example: ['3C273,NGC253', 'IC433,3C279'] sourceflag -- Flag the WVR data for these source(s) as bad and do not produce corrections for it (requires segsource=True) default: [] (none) example: ['3C273'] nsol -- Number of solutions for phase correction coefficients during this observation. By default only one set of coefficients is generated for the entire observation. If more sets are requested, then they will be evenly distributed in time throughout the observation. Values > 1 require segsource=False. default: 1 disperse -- Apply correction for dispersion default: False wvrflag -- Flag the WVR data for these antenna(s) as bad and replace its data with interpolated values default: [] (none) example: ['DV03','DA05','PM02'] statfield -- Compute the statistics (Phase RMS, Disc) on this field only default: '' (all) statsource -- Compute the statistics (Phase RMS, Disc) on this source only default: '' (all) smooth -- Smooth WVR data by this many samples before applying the correction default: 1 (no smoothing) example: 3 scale -- Scale the entire phase correction by this factor default: 1. (no scaling) reversespw -- Reverse the sign of the correction for the listed SPWs (only neede for early ALMA data before Cycle 0) default: '' (none), example: reversespw='0~2,4'; spectral windows 0,1,2,4 cont -- Estimate the continuum (e.g., due to clouds) default: False
Definition at line 8 of file task_wvrgcal.py.
References sdtpimaging_regression.file.
Referenced by wvrgcal.wvrgcal().