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The input data: UV Tables

The main goal of [rgb]1,0,0IMAGER is to convert interferometric measurements stored in uv tables into images suitable for astrophysical interpretation. uv tables contain a set of visibilities. uv tables being the starting point, [rgb]1,0,0IMAGER contains a number of commands to read then and handle them.



Subsections

Gildas manager 2023-06-01