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sd.almacal - Function
5.1.1 Calibration function specific for ALMA data
Description
This method is properly defined for calibration of ALMA data. Input data
must be a scantable object. The calibration scheme is,

where Ta* is an antenna temperature, Tsys is a system temperature, ON and OFF are raw (uncalibrated) spectral data that correspond to on-source and off-source position, respectively. The OFF scan is linearly interpolated in time if it exists in the vicinity of target ON scan. The calmode argument specifies calibration mode. Supported calibration modes are ’ps’ (position switch) and ’fs’ (frequency switch). The ’ps’ includes calibration for nutator switching as well as classical position switching. The ’ps’ mode also supports calibration of OTF position raster scanned data that consists of on-source scans with simple scan pattern and explicit off-source scans.
Arguments
Inputs |
| ||
scantab |
| input data as a scantable
| |
| allowed: | scantable | |
| Default: | ||
scannos |
| a list of scan numbers to be calibrated
| |
| allowed: | (list of) integer, string |
|
| Default: | [] (all data) |
|
calmode |
| Calibration mode
| |
| allowed: | string (’ps’, ’fs’, ’none’) |
|
| Default: | ’none’ |
|
verify |
| Verify calibration if True
| |
| allowed: | bool |
|
| Default: | False |
|
scantable
Example
scal=sd.almacal(s,calmode=’ps’)
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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