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simulator.corrupt - Function
2.4.1 Corrupt the data with visibility errors
Description
Add errors specified by the set functions (such as noise, gains, polarization
leakage, bandpass, etc) to the visibility data. The errors are applied to the
MODEL_DATA, and written to the DATA and CORRECTED_DATA
columns. Note that corrupt handles only visibility-plane effects, not
image-plane effects such as pointing errors and voltage patterns, which get
applied in predict. Note, the function applies errors to both cross- and
auto-correlation data; The auto-correlation data are corrupted properly only
for the thermalnoise set by setnoise. NOTE: sm.predict assumes the model
image units are Jy/pixel, and in fact will overwrite the brightness units of the
image itself!
Arguments
bool
Example
sm,openfromms(’3C273XC1.MS’);
sm.predict(’3C273XC1.FAKE.IMAGE’);
sm.setnoise( mode=’simplenoise’, simplenoise=’0.1Jy’);
sm.setpa( mode=’calculate’);
sm.corrupt();
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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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