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8.3.4.4 Calibration of GBT data
Data from the GBT are uncalibrated and come as sets of integrations representing the different phases of a calibration cycle (e.g., on source, calibration on, on source, calibration off, on reference, calibration on; on reference, calibration off). Currently, there are a number of routines emulating the standard GBT calibration (in GBTIDL):
- calps - calibrate position switched data
- calfs - calibrate frequency switched data
- calnod - calibration nod (beam switch) data
All these routines calibrate the spectral data to antenna temperature adopting the GBT calibration method as described in the GBTIDL calibration document available at:
There are two basic steps:
First, determine system temperature using a noise tube calibrator (sd.dototalpower())
For each integration, the system temperature is calculated from CAL noise on/off data as:
Tsys = Tcal × +
ref which refers to reference data and the spectral data are averaged across the bandpass. Note that the central 80% of the spectra are used for the calculation.
Second, determine antenna temperature (sd.dosigref())
The antenna temperature for each channel is calculated as:
Ta(ν) = Tsys ×
where sig = (sigcalon + sigcaloff), ref =
(refcalon + refcaloff).
Each calibration routine may be used as:
calibrated_scans = sd.calps(scans,[scanlist]) # calibrate scantable with position-switched
# scheme
Note: For calps and calnod, the scanlist must be scan pairs in correct order as these routines only do minimal checking.
More information about CASA may be found at the
CASA web page
Copyright © 2010 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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