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2.2.1 Specialization of setsolve for cubic spline G (time-dependent gain)
solving
Description
This function is a specialization of the setsolve method which should be used
when cubic spline G solutions are desired, e.g., when SNR on calibrators is
very low. Currently, this solving mode treats dual polarization data on a
per-polarization basis. The option to obtain a joint solution (a la ’T’) will be
provided in the future.
The visibility data are averaged in frequency (for multi-channel data) prior to the solution.
This method uses many of the basic parameters as the generic setsolve. Parameters unique to the spline solver are:
Pending improvements:
Arguments
| Inputs |
| ||
| table |
| Output calibration table name
| |
| allowed: | string |
|
| Default: |
| |
| append |
| Append to existing table?
| |
| allowed: | bool | |
| Default: | false |
|
| mode |
| Phase or Amplitude mode?
| |
| allowed: | string |
|
| Default: | AMP PHASAMP PHAS |
|
| splinetime |
| Spline timescale (sec)
| |
| allowed: | double |
|
| Default: | 10800 |
|
| preavg |
| Pre-averaging interval (in sec)
| |
| allowed: | double |
|
| Default: | 0.0 |
|
| npointaver |
| ||
| allowed: | int |
|
| Default: | 10 |
|
| phasewrap |
| ||
| allowed: | double |
|
| Default: | 250 |
|
| refant |
| Reference antenna. Default is none.
| |
| allowed: | any |
|
| Default: | variant |
|
Example
In this example, a spline solution is first found for phase on a hourly timescale, then for amplitude on a three-hour timescale.
Please send any comments or questions about CASA or AIPS++ to aips2-requests@nrao.edu
Copyright © 2008 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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Updated daily during alpha development.