WorkshopSelfcal: Difference between revisions
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Self-calibration can also be used to improve your spectral line imaging. | Self-calibration can also be used to improve your spectral line imaging. | ||
== More Advanced Applications == | |||
Revision as of 14:43, 28 November 2011
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
Overview
Data Description
You will use the now-familiar NGC 3256 Band 3 or TW Hydra Band 7 Science Verification data.
Recommended Approach
Continuum Self Calibration
Continuum-to-Line Self Calibration
Self-calibration can also be used to improve your spectral line imaging.
