JP-3677: Add maximum_shower_amplitude parameter to jump step #8890
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Not sure why I can't request a review, but tagging @kmacdonald-stsci |
Codecov ReportAll modified and coverable lines are covered by tests ✅
Additional details and impacted files@@ Coverage Diff @@
## main #8890 +/- ##
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- Coverage 63.68% 63.62% -0.06%
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Files 375 375
Lines 38691 38692 +1
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- Hits 24640 24619 -21
- Misses 14051 14073 +22 ☔ View full report in Codecov by Sentry. |
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Updated to catch additional runtime warnings, and ensure the maximum amplitude is passed in the correct units so that it works for both FAST and SLOW mode data. |
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This PR addresses JP-3677 by adding a maximum_shower_amplitude parameter to the MIRI cosmic ray showers code, and ensuring that any changes in the rate image due to shower flagging are below this amplitude.
See also corresponding stcal PR spacetelescope/stcal#306
Tasks
Build 11.3(use the latest build if not sure)no-changelog-entry-needed)changes/:echo "changed something" > changes/<PR#>.<changetype>.rst(see below for change types)docs/pageokify_regteststo update the truth filesnews fragment change types...
changes/<PR#>.general.rst: infrastructure or miscellaneous changechanges/<PR#>.docs.rstchanges/<PR#>.stpipe.rstchanges/<PR#>.datamodels.rstchanges/<PR#>.scripts.rstchanges/<PR#>.fits_generator.rstchanges/<PR#>.set_telescope_pointing.rstchanges/<PR#>.pipeline.rststage 1
changes/<PR#>.group_scale.rstchanges/<PR#>.dq_init.rstchanges/<PR#>.emicorr.rstchanges/<PR#>.saturation.rstchanges/<PR#>.ipc.rstchanges/<PR#>.firstframe.rstchanges/<PR#>.lastframe.rstchanges/<PR#>.reset.rstchanges/<PR#>.superbias.rstchanges/<PR#>.refpix.rstchanges/<PR#>.linearity.rstchanges/<PR#>.rscd.rstchanges/<PR#>.persistence.rstchanges/<PR#>.dark_current.rstchanges/<PR#>.charge_migration.rstchanges/<PR#>.jump.rstchanges/<PR#>.clean_flicker_noise.rstchanges/<PR#>.ramp_fitting.rstchanges/<PR#>.gain_scale.rststage 2
changes/<PR#>.assign_wcs.rstchanges/<PR#>.badpix_selfcal.rstchanges/<PR#>.msaflagopen.rstchanges/<PR#>.nsclean.rstchanges/<PR#>.imprint.rstchanges/<PR#>.background.rstchanges/<PR#>.extract_2d.rstchanges/<PR#>.master_background.rstchanges/<PR#>.wavecorr.rstchanges/<PR#>.srctype.rstchanges/<PR#>.straylight.rstchanges/<PR#>.wfss_contam.rstchanges/<PR#>.flatfield.rstchanges/<PR#>.fringe.rstchanges/<PR#>.pathloss.rstchanges/<PR#>.barshadow.rstchanges/<PR#>.photom.rstchanges/<PR#>.pixel_replace.rstchanges/<PR#>.resample_spec.rstchanges/<PR#>.residual_fringe.rstchanges/<PR#>.cube_build.rstchanges/<PR#>.extract_1d.rstchanges/<PR#>.resample.rststage 3
changes/<PR#>.assign_mtwcs.rstchanges/<PR#>.mrs_imatch.rstchanges/<PR#>.tweakreg.rstchanges/<PR#>.skymatch.rstchanges/<PR#>.exp_to_source.rstchanges/<PR#>.outlier_detection.rstchanges/<PR#>.tso_photometry.rstchanges/<PR#>.stack_refs.rstchanges/<PR#>.align_refs.rstchanges/<PR#>.klip.rstchanges/<PR#>.spectral_leak.rstchanges/<PR#>.source_catalog.rstchanges/<PR#>.combine_1d.rstchanges/<PR#>.ami.rstother
changes/<PR#>.wfs_combine.rstchanges/<PR#>.white_light.rstchanges/<PR#>.cube_skymatch.rstchanges/<PR#>.engdb_tools.rstchanges/<PR#>.guider_cds.rst