National Radio
Astronomy Observatory

1.6.3.8 Splitting the Data

After a suitable calibration is achieved, it may be desirable to create one or more new measurement sets containing the data for selected sources. This can be done using the split task (§ 4.7.1).

Further imaging and calibration (e.g. self-calibration) can be carried out on these split Measurement Sets.

More information about CASA may be found at the CASA web page

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