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Version 1.9 Build 1488 |
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Package | bima | |
Module | bimacalibrater | |
Tool | bimacalibrater |
The solve function wraps the calibrater tool's solve function. Solutions are generated and a calibration table is written for the specified sources. In addition, a keyword called SPW_INFO is written to the calibration table. This keyword contains information on the spectral window configuration of the source being solved for. This information is then read by the transfer function to help it make an educated guess about how the windows in the calibration written by solve map to the spectral windows in the sources to which the calibration will be applied.
sources | Nicknames of sources on which to run calibrater.solve() | ||
Allowed: | Vector of strings (nicknames or roles of sources) | ||
Default: | 'phcals' |
- bc := bimacalibrater(['sgrb2.ms','sgra.ms'], + '1733-130.ms',targetnames=['sgrb','sgra'],phcalnames='1733'); - bc.setjy(fluxdensity=[5,0,0,0]); T - bc.setdata('1733',mode='channel'); T - bc.setsolve('1733','G',60,refant=4,table='gcal'); T - # bc.solve('phcals') or bc.solve('1733') are equivalent to the following - bc.solve() T