VLA Data Combination-W49A-CASA6.5.4: Revision history

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    22 February 2024

    • curprev 17:1117:11, 22 February 2024Jkhor talk contribs 30,317 bytes +30,317 Created page with "''This CASA Guide is for Version 6.5.4 of CASA'' == Introduction == A perfect image requires measurement of all spatial scales, which is equivalent to filling in the complete uv plane. Unfortunately, this can never be achieved with an aperture synthesis interferometer, although a large number of baselines, long integration times, and multi-frequency-synthesis are all good approaches to increase the uv-coverage. One method to obtain more baselines is to observe in diffe..."