| Getting Started | Documentation | Glish | Learn More | Programming | Contact Us |
| Version 1.9 Build 803 |
|
For point sources of unknown flux density, but for which valid solutions have been derived against a unit point source model, the absolute flux density can be established by scaling the mean gain amplitudes against those of the known amplitude calibrators. This scaling is achieved using the calibrater.fluxscale function.
In both examples below, the amplitude scale is set with 3C286 as the
reference flux density calibrator. The output calibration table
contains the scaled G calibration factors for all of the transfer
sources, and will be used in subsequent reduction steps. Proper
scaling is indicated in the calibrater.plotcal plots by smoothly varying
(ideally constant) amplitude gains for each antenna, despite
source changes. At high frequencies (
> 15 GHz), this scaling
step may be biased by elevation-dependent variation of the atmospheric
contribution to the system noise temperature. Methods for treating
this case properly will be available in the near future.