AssembleCellCoaddConfig#
- class lsst.drp.tasks.assemble_cell_coadd.AssembleCellCoaddConfig(*args, **kw)#
Bases:
PipelineTaskConfigAttributes Summary
Mask planes that count towards the masked fraction within a cell.
Calculate coadd variance from input variance by stacking statistic.
Field which refers to a dynamically added configuration class which is based on a PipelineTaskConnections class.
Calculate coadd weight from the input warp? Otherwise, the weight is obtained from the visitSummaryList connection.
Coadd the inverse aperture corrections for each cell? This is formally the more accurate way but may be turned off for parity with deepCoadd.
Interpolate over pixels with NO_DATA mask set? (
bool, defaultTrue)Scale warps to a common zero point? This is not needed if they have absolute flux calibration.
Substitute the mask planes input warp with an alternative artifact mask? (
bool, defaultTrue)Task to interpolate (and extrapolate) over pixels with NO_DATA mask on cell coadds (
ConfigurableInstance, default<class 'lsst.pipe.tasks.interpImage.InterpImageConfig'>)Threshold (in fractional weight) of rejection at which we propagate a mask plane to the coadd; that is, we set the mask bit on the coadd if the fraction the rejected frames would have contributed exceeds this value.
Maximum fraction of masked pixels in a cell.
The minimum overlap fraction required for a single (visit, detector) input to be included in a cell.
Number of noise planes to include in the coadd.
Dimensions of the PSF image stamp size to be assigned to cells (must be odd).
Configuration for the warper that warps the PSFs.
Mask planes to remove before coadding (
List, default['NOT_DEBLENDED'])Flag to enable/disable saving of log output for a task, enabled by default.
Task to scale warps to a common zero point Deprecated: Now that visits are scaled to nJy it is no longer necessary or recommended to scale the zero point, so this will be removed after v29.
Attributes Documentation
- bad_mask_planes#
Mask planes that count towards the masked fraction within a cell. (
List, default('BAD', 'NO_DATA', 'SAT', 'CLIPPED'))
- calc_error_from_input_variance#
Calculate coadd variance from input variance by stacking statistic. Passed to AccumulatorMeanStack. (
bool, defaultTrue)
- connections: pexConfig.ConfigField#
Field which refers to a dynamically added configuration class which is based on a PipelineTaskConnections class.
- do_calculate_weight_from_warp#
Calculate coadd weight from the input warp? Otherwise, the weight is obtained from the visitSummaryList connection. This is meant as a fallback when run outside the pipeline. (
bool, defaultFalse)
- do_coadd_inverse_aperture_corrections#
Coadd the inverse aperture corrections for each cell? This is formally the more accurate way but may be turned off for parity with deepCoadd. (
bool, defaultFalse)
- do_interpolate_coadd#
Interpolate over pixels with NO_DATA mask set? (
bool, defaultTrue)
- do_scale_zero_point#
Scale warps to a common zero point? This is not needed if they have absolute flux calibration. Deprecated: Now that visits are scaled to nJy it is no longer necessary or recommended to scale the zero point, so this will be removed after v29. (
bool, defaultFalse)
- do_use_artifact_mask#
Substitute the mask planes input warp with an alternative artifact mask? (
bool, defaultTrue)
- interpolate_coadd#
Task to interpolate (and extrapolate) over pixels with NO_DATA mask on cell coadds (
ConfigurableInstance, default<class 'lsst.pipe.tasks.interpImage.InterpImageConfig'>)
- mask_propagation_thresholds#
Threshold (in fractional weight) of rejection at which we propagate a mask plane to the coadd; that is, we set the mask bit on the coadd if the fraction the rejected frames would have contributed exceeds this value. (
Dict, default{'SAT': 0.1})
- max_maskfrac#
Maximum fraction of masked pixels in a cell. This is currently just a placeholder and is not used now (
float, default0.99)Valid Range = [0.0,1.0)
- min_overlap_fraction#
The minimum overlap fraction required for a single (visit, detector) input to be included in a cell. (
float, default1.0)Valid Range = [0.0,1.0]
- num_noise_realizations#
Number of noise planes to include in the coadd. This should not exceed the corresponding config parameter specified in
MakeDirectWarpConfig. (int, default0)
- psf_dimensions#
Dimensions of the PSF image stamp size to be assigned to cells (must be odd). (
int, default35)
- psf_warper#
Configuration for the warper that warps the PSFs. It must have the same configuration used to warp the images. (
WarperConfig, default<class 'lsst.afw.math._warper.WarperConfig'>)
- remove_mask_planes#
Mask planes to remove before coadding (
List, default['NOT_DEBLENDED'])
- saveLogOutput#
Flag to enable/disable saving of log output for a task, enabled by default. (
bool, defaultTrue)
- scale_zero_point#
Task to scale warps to a common zero point Deprecated: Now that visits are scaled to nJy it is no longer necessary or recommended to scale the zero point, so this will be removed after v29. (
ConfigurableInstance, default<class 'lsst.pipe.tasks.scaleZeroPoint.ScaleZeroPointConfig'>)