flint.prefect.flows.subtract_cube_pipeline¶
This is a workflow to subtract a continuum model and image the channel-wise data
Unlike the continuum imaging and self-calibnration pipeline this flow currently expects that all measurement sets are in the flint format, which means other than the naming scheme that they have been been preprocessed to place them in the IAU frame and have had their fields table updated. That is to say that they have already been preprocessed and fixed.
Functions¶
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Verify that the options supplied to run the subtract field options make sense |
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Search for MSs in a directory and, if necessary, perform checks around |
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Search for MSs to image. See |
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Separate flow to perform the potentially expensive model prediction |
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Use the fits-cube package to take all input images and create a single output cube. |
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A single task that internally runs the wsclean imager task while iterates over |
Module Contents¶
- flint.prefect.flows.subtract_cube_pipeline._check_and_verify_options(subtract_field_options: flint.options.SubtractFieldOptions | None = None, addmodel_subtract_field_options: flint.options.AddModelSubtractFieldOptions | None = None, crystalball_subtract_field_options: flint.predict.crystalball.CrystalBallOptions | None = None) None[source]¶
Verify that the options supplied to run the subtract field options make sense
- flint.prefect.flows.subtract_cube_pipeline.find_and_setup_mss(science_path_or_mss: pathlib.Path | tuple[flint.ms.MS, Ellipsis], expected_ms_count: int, data_column: str) tuple[flint.ms.MS, Ellipsis][source]¶
Search for MSs in a directory and, if necessary, perform checks around their consistency. If the input data appear to be collection of MSs already assume they have already been set and checked for consistency.
- Parameters:
science_path_or_mss (Union[Path, List[MS, ...]]) – Path to search or existing MSs
expected_ms_count (int) – Expected number of MSs to find
data_column (str) – The data column to nominate if creating MSs after searching
- Raises:
FrequencyMismatchError – Raised when frequency information is not consistent
- Returns:
Collection of MSs
- Return type:
Tuple[MS, …]
- flint.prefect.flows.subtract_cube_pipeline.find_mss_to_image(mss_parent_path: pathlib.Path, expected_ms_count: int | None = None, data_column: str = 'CORRECTED_DATA', model_column: str = 'MODEL_DATA') tuple[flint.ms.MS, Ellipsis][source]¶
Search for MSs to image. See
flint.ms.find_mssfor further details.- Parameters:
mss_parent_path (Path) – Path to search for MSs in
expected_ms_count (Optional[int], optional) – Expected number of measurement sets to find. Defaults to None.
data_column (str, optional) – The nominated data column that should eb set. Defaults to “CORRECTED_DATA”.
model_column (str, optional) – The nominated model data column that should be set. Defaults to “MODEL_DATA”.
- Returns:
Collect of MSs
- Return type:
Tuple[MS, …]
- flint.prefect.flows.subtract_cube_pipeline.flow_addmodel_to_mss(science_path_or_mss: pathlib.Path | tuple[flint.ms.MS, Ellipsis], addmodel_subtract_field_options: flint.options.AddModelSubtractFieldOptions, expected_ms: int, data_column: str) tuple[flint.ms.MS, Ellipsis][source]¶
Separate flow to perform the potentially expensive model prediction into MSs
- flint.prefect.flows.subtract_cube_pipeline.flow_subtract_cube(science_path: pathlib.Path, subtract_field_options: flint.options.SubtractFieldOptions, addmodel_subtract_field_options: flint.options.AddModelSubtractFieldOptions, crystalball_subtract_field_options: flint.predict.crystalball.CrystalBallOptions) None[source]¶
- flint.prefect.flows.subtract_cube_pipeline.setup_run_subtract_flow(science_path: pathlib.Path, subtract_field_options: flint.options.SubtractFieldOptions, addmodel_subtract_field_options: flint.options.AddModelSubtractFieldOptions, crystalball_subtract_field_options: flint.predict.crystalball.CrystalBallOptions, cluster_config: pathlib.Path) None[source]¶
- flint.prefect.flows.subtract_cube_pipeline.task_combine_all_linmos_images(linmos_commands: list[flint.coadd.linmos.LinmosResult], remove_original_images: bool = False, combine_weights: bool = False, time_domain: bool = False, update_fits_cube_options: dict[str, Any] | None = None) pathlib.Path[source]¶
Use the fits-cube package to take all input images and create a single output cube.
- Parameters:
linmos_commands (list[LinmosResult]) – The output linmos commands to concatenated into a single cube.
remove_original_images (bool, optional) – Remove the original images after the cube has been formed. Defaults to False.
combine_weights (bool, optional) – Whether to concatenated the images or the weights that are described by the input linmos_commands. Defaults to False.
time_domain (bool, optional) – Whether images are to be formed on the spectral or time axis. Defaults to False.
bounding_box (bool, optional) – Whether to trim the output cube to include only valid pixels (see fitscube docs). Defaults to False.
invalidate_zeros (bool, optional) – Where to mark pixels that are exactly zero as invalid (replace with a NaN). Defaults to False.
- Returns:
The output cube path
- Return type:
Path
- flint.prefect.flows.subtract_cube_pipeline.task_map_all_wsclean(in_mss: list[flint.ms.MS], *args, **kwargs) list[flint.imager.wsclean.WSCleanResult][source]¶
A single task that internally runs the wsclean imager task while iterates over the input list of measurement sets when run. It performs the same operation as the prefect task enabled map operator, but unlike the .map method all outputs are tracked in a single prefect task. This is used to lower the load on the prefect server.
- Parameters:
in_mss (list[MS]) – List of measurement sets to image
- Returns:
The list of output wsclean results
- Return type:
list[WSCleanResult]