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DM-41881: Decrease nBins for LATISS focal plane plots in analysis_tools #95

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Dec 3, 2023
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DM-41881: Decrease nBins for LATISS focal plane plots in analysis_tools #95

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38 changes: 33 additions & 5 deletions pipelines/LATISS/DRP.yaml
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Original file line number Diff line number Diff line change
Expand Up @@ -3,18 +3,17 @@ instrument: lsst.obs.lsst.Latiss
imports:
- location: $DRP_PIPE_DIR/pipelines/_ingredients/DRP-full.yaml
- location: $ANALYSIS_TOOLS_DIR/pipelines/coaddColumnValidate.yaml
- location: $ANALYSIS_TOOLS_DIR/pipelines/matchedVisitQualityCore.yaml
- location: $ANALYSIS_TOOLS_DIR/pipelines/coaddQualityCore.yaml
exclude:
- analyzeObjectTableCore
# The following are from analysis_drp
# TODO: remove once they have all been ported to analysis_tools (DM-39081)
- location: $ANALYSIS_DRP_DIR/pipelines/analysis_drp_plots.yaml
include:
- plot_ri_gr_psf
- plot_ri_gr_cmodel
- plot_wFit_PSF
- plot_xFit_PSF
# The following are from analysis_drp
# TODO: remove once they have all been ported to analysis_tools (DM-39081)
- location: $ANALYSIS_DRP_DIR/pipelines/coaddQAPlots_tier2_3.yaml
include:
- plot_ri_gr_contour_psf
Expand Down Expand Up @@ -46,8 +45,8 @@ tasks:
# psf kernel size.
maxPsfFwhm: 1.9

# Importing and defining analyzeObjectTableCore here to omit plots that
# require z and/or y band data.
# Defining analyzeObjectTableCore here to omit plots that require z and/or
# y band data.
analyzeObjectTableCore:
class: lsst.analysis.tools.tasks.ObjectTableTractAnalysisTask
config:
Expand All @@ -67,6 +66,35 @@ tasks:
from lsst.analysis.tools.atools import *
from lsst.analysis.tools.contexts import *

# Defining analyzematchedVisitCore here to change the nBins config and omit
# plots currently not relevant for LATISS imaging.
analyzeMatchedVisitCore:
class: lsst.analysis.tools.tasks.AssociatedSourcesTractAnalysisTask
config:
connections.outputName: matchedVisitCore
atools.stellarPhotometricRepeatability: StellarPhotometricRepeatability
atools.stellarPhotometricResiduals: StellarPhotometricResidualsFocalPlane
atools.stellarPhotometricResiduals.produce.plot.nBins: 80
atools.stellarAstrometricResidualsRA: StellarAstrometricResidualsRAFocalPlanePlot
atools.stellarAstrometricResidualsRA.produce.nBins: 80
atools.stellarAstrometricResidualsDec: StellarAstrometricResidualsDecFocalPlanePlot
atools.stellarAstrometricResidualsDec.produce.nBins: 80
atools.stellarAstrometricResidualStdDevRA: StellarAstrometricResidualStdDevRAFocalPlanePlot
atools.stellarAstrometricResidualStdDevRA.produce.nBins: 80
atools.stellarAstrometricResidualStdDevDec: StellarAstrometricResidualStdDevDecFocalPlanePlot
atools.stellarAstrometricResidualStdDevDec.produce.nBins: 80
# The following are the AMX metrics: median relative astrometric measurement
# error on N arc minute scales from single visit images shall be less than
# this value, where N = 5, 20, 200 arcmin for X = 1, 2, 3, respectivley.
# Given the current distribution of visits/field, one X = 1 is included for
# now (the others just pollute the repo with empty plots). The others can/should
# be added if the observing strategy changes to warrant it.
atools.stellarAstrometricRepeatability1: AstrometricRelativeRepeatability
atools.stellarAstrometricRepeatability1.xValue: 1
atools.stellarAstrometricRepeatability1.process.calculateActions.rms.annulus: 5
python: |
from lsst.analysis.tools.atools import *

subsets:
step1:
subset:
Expand Down