ALMA SIS14 apcal: Difference between revisions

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== Setup ==
== Setup ==


To run this tutorial, you need the measurements set "sis14_ampandphase.ms." This measurement set contains only a quasar (the phase calibrator from the parent data set). If you are using the pre-provided directory structure then you want to work in the direcory
To run this tutorial, you need the measurements set "sis14_ampandphase.ms." This measurement set contains only a quasar (the phase calibrator from the parent data set). If you are using the pre-provided directory structure then you want to work in the directory:
 


<pre style="background-color: #fffacd;">
<pre style="background-color: #fffacd;">
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</pre>
</pre>


and you can copy the data to your working directory using the commands
(relative to the root for the package) and you can copy the data to your working directory using the commands


<source lang="python">
<source lang="python">
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os.system("cp -r ../../working_data/sis14_ampandphase.ms sis14_ampandphase.ms")
os.system("cp -r ../../working_data/sis14_ampandphase.ms sis14_ampandphase.ms")
</source>
</source>
With this measurement set in place, you can follow the tutorial below inside the "basic_cal/" directory.


== Overview ==
== Overview ==

Revision as of 14:42, 28 February 2014

Setup

To run this tutorial, you need the measurements set "sis14_ampandphase.ms." This measurement set contains only a quasar (the phase calibrator from the parent data set). If you are using the pre-provided directory structure then you want to work in the directory:

lessons/basic_cal/

(relative to the root for the package) and you can copy the data to your working directory using the commands

# In CASA
os.system("rm -rf sis14_ampandphase.ms")
os.system("cp -r ../../working_data/sis14_ampandphase.ms sis14_ampandphase.ms")

With this measurement set in place, you can follow the tutorial below inside the "basic_cal/" directory.

Overview

Phase Calibration (per Scan)

First, we calibrate phase as a function of time.

# In CASA
listobs("sis14_ampandphase.ms")

Now we calibrate the phase correction for each antenna as a function of time.

# In CASA
os.system("rm -rf phase.cal")
gaincal(vis="sis14_ampandphase.ms",
        caltable="phase.cal",
        field="0",
        solint="inf",
        calmode="p",
        refant="DV22",
        gaintype="G")

Now we plot the results of the calibration.

# In CASA
plotcal(caltable="phase.cal", 
        xaxis="time",
        yaxis="phase",
        subplot=331,
        iteration="antenna",
        plotrange=[0,0,-180,180])

Amplitude Calibration (per Scan)

Now calibrate the amplitude response of each antenna as a function of time.

# In CASA
os.system("rm -rf amp.cal")
gaincal(vis="sis14_ampandphase.ms",
        caltable="amp.cal",
        field="0",
        solint="inf",
        calmode="a",
        refant="DV22",
        gaintype="G",
        gaintable="phase.cal")

Plot the results of this fit.

# In CASA
plotcal(caltable="amp.cal", 
        xaxis="time",
        yaxis="amp",
        subplot=331,
        iteration="antenna",
        plotrange=[0,0,0,0])

Phase and Amplitude Calibration (per Integration)

We can also solve for the antenna corrections on shorter timescales.

# In CASA
os.system("rm -rf apcal_int.cal")
gaincal(vis="sis14_ampandphase.ms",
        caltable="apcal_int.cal",
        field="0",
        solint="int",
        calmode="ap",
        refant="DV22",
        gaintype="G")

Plot the per-integration variation of the phase.

# In CASA
plotcal(caltable="apcal_int.cal", 
        xaxis="time",
        yaxis="phase",
        subplot=331,
        iteration="antenna",
        plotrange=[0,0,-180,180])

Now plot the per-integration variation of the amplitude.

# In CASA
plotcal(caltable="apcal_int.cal", 
        xaxis="time",
        yaxis="amp",
        subplot=331,
        iteration="antenna",
        plotrange=[0,0,0,0])

Advanced Considerations

Averaging Options

"Layering" Calibrations

Removing Short-Timescale Phase Variations Before Amplitude Calibration?