Sky components
ska_sdp_func_python.sky_component.operations Module
Functions to manage sky components operations.
Functions
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Apply a primary beam to a SkyComponent. |
Apply a voltage pattern to a SkyComponent. |
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Filter sky components by stokes I flux. |
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Find the nearest component to a given direction. |
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Find the nearest component in a list to a given direction (home). |
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Find the matrix of separations for two lists of components. |
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Find gaussian components in Image above a certain threshold as SkyComponent. |
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Match a list of candidates to a reference set of SkyComponents. |
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Match a list of candidates to a reference set of SkyComponents. |
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Fit a two-dimensional Gaussian skycomponent using astropy.modeling. |
Fit the spectral index for a multi frequency SkyComponent. |
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Iterate through Voronoi decomposition, returning a generator yielding fullsize images. |
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Insert a SkyComponent into an Image. |
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Partition sky components by nearest target source. |
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Remove the faintest of a pair of components that are within a specified distance. |
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Select components with a range in separation. |
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Assign components to nearest in the target. |
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Construct a Voronoi decomposition of a set of components. |
ska_sdp_func_python.sky_component.taylor_terms Module
SkyComponent functions using taylor terms in frequency.
Functions
Calculate frequency taylor terms for a List of SkyComponents. |
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Find skycomponents by fitting to moment0, fit polynomial in frequency, return in frequency space. |
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Gather a SkyComponent list from [chan][source] to [source]. |
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Smooth SkyComponent fluxes by fitting polynomial in frequency. |
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Transpose a SkyComponent list from [source,chan] to [chan,source]. |