WorkshopSelfcal: Difference between revisions

Revision as of 18:41, 28 November 2011

You will use the now-familiar NGC 3256 Band 3 or TW Hydra Band 7 Science Verification data.

Self-calibration can also be used to improve your spectral line imaging.

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	This page describes the hands-on self calibration portion of the ALMA data reduction workshop. In this session you will carry out self-calibration on ALMA Science Verification data to improve the image quality. This page describes the data and introduces the scripts. It is not a full-fledged CASA guide, only background for the hands on portion of the workshop. For the imaging session in the morning go here: [[WorkshopImaging]]

	== Data Description ==		== Data Description ==