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NRAO Home > CASA > CASA Task Reference Manual |
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0.1.139 wvrgcal
Requires:
Synopsis
Generate a gain table based on Water Vapour Radiometer data
Description
Information about the observation and the performance of WVRGCAL is
written to the CASA logger and also returned in a dictionary; see the CASA
cookbook for a more detailed description of these parameters. The dictionary
element ’success’ is True if no errors occured.
Of particular note is the discrepancy parameter (Disc): high values (¿ a few hundred microns) may indicate some levels of cloud contamination and the effect of applying the WVRGCAL correction should be checked; values ¿ 1000 um in all antennas have currently been found to indicate that WVRGCAL correction should not be used.
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: 0 (ALMA default for cycle 1, for cycle 0, i.e. up to Jan 2013 it was -1)
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 – Regard the WVR data for these antenna(s) as bad and use interpolated values instead 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 the calibration solution on the given timescale default: ” (no smoothing), example: ’3s’ smooth on a timescale of 3 seconds
scale – Scale the entire phase correction by this factor default: 1. (no scaling)
spw – List of the spectral window IDs for which solutions should be saved into the caltable default: [] (all spectral windows), example [17,19,21,23]
wvrspw – List of the spectral window IDs from which the WVR data should be taken default: [] (all WVR spectral windows), example [0]
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
maxdistm – maximum distance (m) an antenna may have to be considered for being part of the antenna set (minnumants to 3 antennas) for the interpolation of a solution for a flagged antenna default: 500.
minnumants – minimum number of near antennas required for interpolation default: 2
mingoodfrac – If the fraction of unflagged data for an antenna is below this value (0. to 1.), the antenna is flagged. default: 0.8
usefieldtab – derive the antenna AZ/EL values from the FIELD rather than the POINTING table default: False
refant – use the WVR data from this antenna for calculating the dT/dL parameters (can give ranked list) default: ” (use the first good or interpolatable antenna), examples: ’DA45’ - use DA45 [’DA45’,’DV51’] - use DA45 and if that is not good, use DV51 instead
offsetstable – (experimental) subtract the temperature offsets in this table from the WVR measurements before using them to calculate the phase corrections default: ” (do not apply any offsets) examples: ’uid___A002_Xabd867_X2277.cloud_offsets’ use the given table
Arguments
Inputs |
| ||
vis |
| Name of input visibility file
| |
| allowed: | string |
|
| Default: |
| |
caltable |
| Name of output gain calibration table
| |
| allowed: | string |
|
| Default: |
|
|
toffset |
| Time offset (sec) between interferometric and WVR data
| |
| allowed: | double | |
| Default: | 0 |
|
segsource |
| Do a new coefficient calculation for each source
| |
| allowed: | bool | |
| Default: | True |
|
sourceflag |
| Regard the WVR data for these source(s) as bad and do
not produce corrections for it (requires segsource=True)
| |
| allowed: | stringArray |
|
| Default: |
| |
tie |
| Prioritise tieing the phase of these sources as well as
possible (requires segsource=True)
| |
| allowed: | stringArray |
|
| Default: |
| |
nsol |
| Number of solutions for phase correction coefficients
(nsol>1 requires segsource=False)
| |
| allowed: | int | |
| Default: | 1 |
|
disperse |
| Apply correction for dispersion
| |
| allowed: | bool | |
| Default: | False |
|
wvrflag |
| Regard the WVR data for these antenna(s) as bad
and replace its data with interpolated values from
neighbouring antennas
| |
| allowed: | stringArray |
|
| Default: |
|
|
statfield |
| Compute the statistics (Phase RMS, Disc) on this field
only
| |
| allowed: | string |
|
| Default: |
|
|
statsource |
| Compute the statistics (Phase RMS, Disc) on this source
only
| |
| allowed: | string |
|
| Default: |
| |
smooth |
| Smooth calibration solution on the given timescale
| |
| allowed: | string |
|
| Default: |
| |
scale |
| Scale the entire phase correction by this factor
| |
| allowed: | double |
|
| Default: | 1. |
|
spw |
| List of the spectral window IDs for which solutions
should be saved into the caltable
| |
| allowed: | intArray |
|
| Default: |
|
|
wvrspw |
| List of the spectral window IDs from which the WVR
data should be taken
| |
| allowed: | intArray |
|
| Default: |
|
|
reversespw |
| Reverse the sign of the correction for the listed SPWs
(only needed for early ALMA data before Cycle 0)
| |
| allowed: | string |
|
| Default: |
|
|
cont |
| Estimate the continuum (e.g., due to clouds)
(experimental)
| |
| allowed: | bool |
|
| Default: | False |
|
maxdistm |
| maximum distance (m) of an antenna used for
interpolation for a flagged antenna
| |
| allowed: | double |
|
| Default: | 500. |
|
minnumants |
| minimum number of near antennas (up to 3) required
for interpolation
| |
| allowed: | int |
|
| Default: | 2 |
|
mingoodfrac |
| If the fraction of unflagged data for an antenna is below
this value (0. to 1.), the antenna is flagged.
| |
| allowed: | double |
|
| Default: | 0.8 |
|
usefieldtab |
| derive the antenna AZ/EL values from the FIELD rather
than the POINTING table
| |
| allowed: | bool |
|
| Default: | False |
|
refant |
| use the WVR data from this antenna for calculating the
dT/dL parameters (can give ranked list)
| |
| allowed: | stringArray |
|
| Default: |
|
|
offsetstable |
| (experimental) subtract the temperature offsets in this
table from the WVR measurements before calculating
the phase corrections
| |
| allowed: | string |
|
| Default: |
|
|
variant
Example
wvrgcal(vis=’uid___A002_X1d54a1_X5.ms’, caltable=’cal-wvr-uid___A002_X1d54a1_X5.W’,
toffset=-1, segsource=True, tie=[’Titan,1037-295,NGC3256’], statsource=’1037-295’)
More information about CASA may be found at the
CASA web page
Copyright © 2016 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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