The input data: UV Tables
Keywords: imager

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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

- In a nutshell
- UV table description
  - UV table data format
  - uv header
- NOEMA: UV Tables from CLIC
- ALMA: UV Tables from CASA
  - On the CASA side
  - On the [rgb]1,0,0IMAGER side
  - Current assumptions and limitations
- Reading UV tables
- UV Table handling