Visibility
ska_sdp_func_python.visibility.base Module
Base simple visibility operations, placed here to avoid circular dependencies.
Functions
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Calculate the phasor for a component for a Visibility. |
Recalculate the uvw_lambda values. |
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Phase rotate from the current phase centre to a new phase centre. |
ska_sdp_func_python.visibility.operations Module
Visibility operations
Functions
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Concatenate a list of Visibility's in frequency. |
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Concatenate a list of visibilities. |
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Subtract model_vis from vis, returning new visibility. |
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Fit and remove continuum visibility. |
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Divide visibility by model forming visibility for equivalent point source. |
Integrate visibility across all channels, returning new visibility. |
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Average visibility by groups of channels, returning list of new visibility. |
Convert the polarisation frame data into Stokes parameters. |
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Convert the polarisation frame data into Stokes I dropping other polarisations, return new Visibility. |
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Convert the Stokes I into full polarisation, return new Visibility. |
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Expand number of polarizations to four Optionally change the data type |
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Shrink number of polarizations to nr_polarizations Optionally change the data type |
ska_sdp_func_python.visibility.visibility_geometry Module
Functions for calculating the geometry of a Visibility.
Functions
Return az el for a location, utc_time, and direction. |
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Return hour angles for location, utc_time, and direction. |
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Return parallactic angles for location, utc_time, and direction. |
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Find the UTC time of the nearest transit. |