autowisp.processing_steps.fit_star_shape module

Class Inheritance Diagram

Fit a model for the shape of stars (PSF or PRF) in images.

class autowisp.processing_steps.fit_star_shape.SourceListCreator(*, catalog_sources, fit_variables, grouping, grouping_frame=None, discard_faint=False, remove_group_id=None, **dr_path_substitutions)

Bases: object

Class for creating PRF fitting source lists for a single frame.

__call__(frame_fname)

Return the fitpsf/fitprf source list for this frame.

Parameters:

frame_fname – The filename of the frame to get PRF fitting sources of.

Returns:

The values of all source variables PSF/PRF fitting will use for each fitting group. Each entry is suitable as input to FitStarShape.fit(), with only one fitting group enabled.

Return type:

[numpy record array]

__init__(*, catalog_sources, fit_variables, grouping, grouping_frame=None, discard_faint=False, remove_group_id=None, **dr_path_substitutions)

Set up to create source lists for PSF/PRF fitting.

Parameters:

• catalog_fname – The filename containing a list of catalog sources to fit the shape and measure the brightness of.

• extra_fit_variables – See –map-variables command line argument.

• grouping – A splitting of the input sources in groups, each of which is enabled separately during PRF fitting. Should be a callable taking the input projected sources, catalog information, frame header and extra fit variables and returning A numpy integer array indicating for each source the PRF fitting group it is in. Sources assigned to negative group IDs are never enabled.

• grouping_frame – If None, grouping is derived for each input frames separately, potentially resulting in a different set of sources enabled for each frame. If not None, it should specify the filename of a FITS frame on which to derive the grouping once and all subsequent fits are based on the same exact sources, regardless of where on the frame they appear, as long as they are within the frame.

• discard_faint – See –discard-faint command line argument.

• remove_group_id – See ‘–remove-group-id’ command line argument.

• dr_path_substitutions – Any keywords needed to specify unique paths in the data reduction files for the inputs and output required for shape fitting.

Returns:

None

_group_and_flag_in_frame(header)

Return the group each source belongs to and flag for is source in frame.

Parameters:

header – The FITS header of the frame being fit.

Returns:

The group index for each source

numpy.array(bool):

True iff the source center is inside the frame boundaries

Return type:

numpy.array(int)

_project_sources(header)

Add to self._sources the projected positions and extra fit variables.

Parameters:

header – The header of the FITS frame currently being processed.

Returns:

None

autowisp.processing_steps.fit_star_shape.add_background_options(parser)

Add options configuring the background extraction.

autowisp.processing_steps.fit_star_shape.add_fitting_options(parser)

Add options controlling the fitting process.

autowisp.processing_steps.fit_star_shape.add_grouping_options(parser)

Add options controlling splitting of sources into fitting groups.

autowisp.processing_steps.fit_star_shape.add_shape_options(parser)

Add options defining how the PSF/PRF shape will be modeled.

autowisp.processing_steps.fit_star_shape.add_source_selction_options(parser)

Add options configuring the selection of sources for fitting.

autowisp.processing_steps.fit_star_shape.cleanup_interrupted(interrupted, configuration)

Remove star shape fit datasets from the DR file of the given image.

autowisp.processing_steps.fit_star_shape.create_source_list_creator(dr_fnames, configuration, catalog_lock)

Return a fully configured instance of SourceListCreator.

autowisp.processing_steps.fit_star_shape.fit_frame_set(frame_filenames, configuration, mark_start, mark_end, catalog_lock=<contextlib.nullcontext object>)

Perform a simultaneous fit of all frames included in frame_filenames.

Parameters:

• frame_filenames ([str]) – The list of FITS file containting calibrated frames to fit. The files must include at least 3 extensions: the calibrated pixel values, estimated errors for the pixel values and the pixel quality mask.

• configuration (dict) – The configuration to use for PSF/PRF fitting, background extraction etc.

• mark_start (callable) – Called for each frame in the set before processing begins.

• mark_end (callable) – Called for each frame in the set after processing ends.

Returns:

None

autowisp.processing_steps.fit_star_shape.fit_star_shape(image_collection, start_status, configuration, mark_start, mark_end)

Find the best-fit model for the PSF/PRF in the given images.

autowisp.processing_steps.fit_star_shape.get_dr_substitutions(configuration)

Return the substitutions to use for DR file paths.

autowisp.processing_steps.fit_star_shape.get_shape_fitter_config(configuration)

Return a fully configured instance of FitStarShape.

autowisp.processing_steps.fit_star_shape.has_astrometry(image_fname, substitutions)

Check if the DR file contains a sky-to-frame transformation.

autowisp.processing_steps.fit_star_shape.main()

Run the step for fitting star shapes from the command line.

autowisp.processing_steps.fit_star_shape.parse_command_line(*args)

Return the parsed command line arguments.

autowisp.processing_steps.fit_star_shape.parse_grid_arg(grid_str)

Parse the string specifying the grid on which to model PSF/PRF.