Inheritance diagram for lsst.fgcmcal.fgcmFitCycle.FgcmFitCycleConfig:
Public Member Functions | |
| def | setDefaults (self) |
| def | validate (self) |
Detailed Description
Config for FgcmFitCycle
Definition at line 57 of file fgcmFitCycle.py.
Member Function Documentation
◆ setDefaults()
| def lsst.fgcmcal.fgcmFitCycle.FgcmFitCycleConfig.setDefaults | ( | self | ) |
Definition at line 634 of file fgcmFitCycle.py.
◆ validate()
| def lsst.fgcmcal.fgcmFitCycle.FgcmFitCycleConfig.validate | ( | self | ) |
Definition at line 637 of file fgcmFitCycle.py.
Member Data Documentation
◆ aperCorrFitNBins
|
static |
Initial value:
= pexConfig.Field(
doc=("Number of aperture bins used in aperture correction fit. When set to 0"
"no fit will be performed, and the config.aperCorrInputSlopes will be "
"used if available."),
dtype=int,
default=10,
)
Definition at line 401 of file fgcmFitCycle.py.
◆ aperCorrInputSlopeDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification of aperture correction input slope parameters. These "
"are used on the first fit iteration, and aperture correction parameters will "
"be updated from the data if config.aperCorrFitNBins > 0. It is recommended "
"to set this when there is insufficient data to fit the parameters (e.g. "
"tract mode)."),
keytype=str,
itemtype=float,
default={},
)
Definition at line 420 of file fgcmFitCycle.py.
◆ aperCorrInputSlopes
|
static |
Initial value:
= pexConfig.ListField(
doc=("Aperture correction input slope parameters. These are used on the first "
"fit iteration, and aperture correction parameters will be updated from "
"the data if config.aperCorrFitNBins > 0. It is recommended to set this"
"when there is insufficient data to fit the parameters (e.g. tract mode). "
"If set, must be same length as config.bands, and matched band-by-band."),
dtype=float,
default=[],
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use aperCorrInputSlopeDict instead."),
)
Definition at line 408 of file fgcmFitCycle.py.
◆ applyRefStarColorCuts
|
static |
Initial value:
= pexConfig.Field(
doc="Apply color cuts to reference stars?",
dtype=bool,
default=True,
)
Definition at line 121 of file fgcmFitCycle.py.
◆ approxThroughput
|
static |
Initial value:
= pexConfig.ListField(
doc=("Approximate overall throughput at start of calibration observations. "
"May be 1 element (same for all bands) or the same length as config.bands."),
dtype=float,
default=(1.0, ),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use approxThroughputDict instead."),
)
Definition at line 475 of file fgcmFitCycle.py.
◆ approxThroughputDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification of the approximate overall throughput at the start of "
"calibration observations. Must have one entry per band. Typically should "
"be 1.0."),
keytype=str,
itemtype=float,
default={},
)
Definition at line 484 of file fgcmFitCycle.py.
◆ autoHighCutNSig
|
static |
Initial value:
= pexConfig.Field(
doc=("Number of sigma for automatic computation of (high) outlier cut. "
"Cut is based on exposure gray width (per band), unless "
"useRepeatabilityForExpGrayCuts is set, in which case the star "
"repeatability is used (also per band)."),
dtype=float,
default=4.0,
)
Definition at line 614 of file fgcmFitCycle.py.
◆ autoPhotometricCutNSig
|
static |
Initial value:
= pexConfig.Field(
doc=("Number of sigma for automatic computation of (low) photometric cut. "
"Cut is based on exposure gray width (per band), unless "
"useRepeatabilityForExpGrayCuts is set, in which case the star "
"repeatability is used (also per band)."),
dtype=float,
default=3.0,
)
Definition at line 606 of file fgcmFitCycle.py.
◆ bands
|
static |
Initial value:
= pexConfig.ListField(
doc="Bands to run calibration",
dtype=str,
default=[],
)
Definition at line 60 of file fgcmFitCycle.py.
◆ brightObsGrayMax
|
static |
Initial value:
= pexConfig.Field(
doc="Maximum gray extinction to be considered bright observation",
dtype=float,
default=0.15,
)
Definition at line 297 of file fgcmFitCycle.py.
◆ ccdGrayFocalPlaneChebyshevOrder
|
static |
Initial value:
= pexConfig.Field(
doc="Order of the 2D chebyshev polynomials for focal plane fit.",
dtype=int,
default=3,
)
Definition at line 234 of file fgcmFitCycle.py.
◆ ccdGrayFocalPlaneDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on whether to compute focal-plane residual "
"('ccd gray') corrections."),
keytype=str,
itemtype=bool,
default={},
)
Definition at line 220 of file fgcmFitCycle.py.
◆ ccdGrayFocalPlaneFitMinCcd
|
static |
Initial value:
= pexConfig.Field(
doc=("Minimum number of 'good' CCDs required to perform focal-plane "
"gray corrections. If there are fewer good CCDs then the gray "
"correction is computed per-ccd."),
dtype=int,
default=1,
)
Definition at line 227 of file fgcmFitCycle.py.
◆ ccdGrayMaxStarErr
|
static |
Initial value:
= pexConfig.Field(
doc=("Maximum error on a star observation to use in ccd gray (achromatic residual) "
"computation"),
dtype=float,
default=0.10,
)
Definition at line 469 of file fgcmFitCycle.py.
◆ ccdGraySubCcd
|
static |
Initial value:
= pexConfig.Field(
doc="Compute CCD gray terms on sub-ccd scale",
dtype=bool,
default=False,
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use ccdGraySubCcdDict instead."),
)
Definition at line 194 of file fgcmFitCycle.py.
◆ ccdGraySubCcdChebyshevOrder
|
static |
Initial value:
= pexConfig.Field(
doc="Order of the 2D chebyshev polynomials for sub-ccd gray fit.",
dtype=int,
default=1,
)
Definition at line 209 of file fgcmFitCycle.py.
◆ ccdGraySubCcdDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on whether to compute achromatic per-ccd residual "
"('ccd gray') on a sub-ccd scale."),
keytype=str,
itemtype=bool,
default={},
)
Definition at line 202 of file fgcmFitCycle.py.
◆ ccdGraySubCcdTriangular
|
static |
Initial value:
= pexConfig.Field(
doc=("Should the sub-ccd gray chebyshev matrix be triangular to "
"suppress high-order cross terms?"),
dtype=bool,
default=True,
)
Definition at line 214 of file fgcmFitCycle.py.
◆ coatingMjds
|
static |
Initial value:
= pexConfig.ListField(
doc="Mirror coating dates in MJD",
dtype=float,
default=(0.0,),
)
Definition at line 574 of file fgcmFitCycle.py.
◆ colorSplitBands
|
static |
Initial value:
= pexConfig.ListField(
doc="Band names to use to split stars by color. Must have 2 entries.",
dtype=str,
length=2,
default=('g', 'i'),
)
Definition at line 540 of file fgcmFitCycle.py.
◆ colorSplitIndices
|
static |
Initial value:
= pexConfig.ListField(
doc="Band indices to use to split stars by color",
dtype=int,
default=None,
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use colorSplitBands instead."),
)
Definition at line 532 of file fgcmFitCycle.py.
◆ cycleNumber
|
static |
Initial value:
= pexConfig.Field(
doc=("FGCM fit cycle number. This is automatically incremented after each run "
"and stage of outlier rejection. See cookbook for details."),
dtype=int,
default=None,
)
Definition at line 239 of file fgcmFitCycle.py.
◆ deltaMagBkgOffsetPercentile
|
static |
Initial value:
= pexConfig.Field(
doc=("Percentile brightest stars on a visit/ccd to use to compute net "
"offset from local background subtraction."),
dtype=float,
default=0.25,
)
Definition at line 258 of file fgcmFitCycle.py.
◆ deltaMagBkgPerCcd
|
static |
Initial value:
= pexConfig.Field(
doc=("Compute net offset from local background subtraction per-ccd? "
"Otherwise, use computation per visit."),
dtype=bool,
default=False,
)
Definition at line 264 of file fgcmFitCycle.py.
◆ doReferenceCalibration
|
static |
Initial value:
= pexConfig.Field(
doc="Use reference catalog as additional constraint on calibration",
dtype=bool,
default=True,
)
Definition at line 105 of file fgcmFitCycle.py.
◆ epochMjds
|
static |
Initial value:
= pexConfig.ListField(
doc="Epoch boundaries in MJD",
dtype=float,
default=(0.0,),
)
Definition at line 280 of file fgcmFitCycle.py.
◆ expGrayErrRecoverCut
|
static |
Initial value:
= pexConfig.Field(
doc=("Maximum exposure gray error to be able to recover bad ccds via interpolation. "
"Visits with more gray variance will only get CCD zeropoints if there are "
"sufficient star observations (minStarPerCcd) on that CCD."),
dtype=float,
default=0.05,
)
Definition at line 394 of file fgcmFitCycle.py.
◆ expGrayHighCut
|
static |
Initial value:
= pexConfig.ListField(
doc=("Maximum (positive) exposure gray for a visit to be considered photometric. "
"Must be same length as config.bands, and matched band-by-band."),
dtype=float,
default=(0.0,),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use expGrayHighCutDict instead."),
)
Definition at line 354 of file fgcmFitCycle.py.
◆ expGrayHighCutDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on maximum (positive) achromatic exposure residual "
"('gray term') for a visit to be considered photometric. Must have one "
"entry per band. Broad-band filters should be 0.2."),
keytype=str,
itemtype=float,
default={},
)
Definition at line 363 of file fgcmFitCycle.py.
◆ expGrayInitialCut
|
static |
Initial value:
= pexConfig.Field(
doc=("Maximum exposure/visit gray value for initial selection of possible photometric "
"observations."),
dtype=float,
default=-0.25,
)
Definition at line 331 of file fgcmFitCycle.py.
◆ expGrayPhotometricCut
|
static |
Initial value:
= pexConfig.ListField(
doc=("Maximum (negative) exposure gray for a visit to be considered photometric. "
"Must be same length as config.bands, and matched band-by-band."),
dtype=float,
default=(0.0,),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use expGrayPhotometricCutDict instead."),
)
Definition at line 337 of file fgcmFitCycle.py.
◆ expGrayPhotometricCutDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on maximum (negative) achromatic exposure residual "
"('gray term') for a visit to be considered photometric. Must have one "
"entry per band. Broad-band filters should be -0.05."),
keytype=str,
itemtype=float,
default={},
)
Definition at line 346 of file fgcmFitCycle.py.
◆ expGrayRecoverCut
|
static |
Initial value:
= pexConfig.Field(
doc=("Maximum (negative) exposure gray to be able to recover bad ccds via interpolation. "
"Visits with more gray extinction will only get CCD zeropoints if there are "
"sufficient star observations (minStarPerCcd) on that CCD."),
dtype=float,
default=-1.0,
)
Definition at line 371 of file fgcmFitCycle.py.
◆ expVarGrayPhotometricCut
|
static |
Initial value:
= pexConfig.Field(
doc="Maximum exposure variance to be considered possibly photometric",
dtype=float,
default=0.0005,
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use expVarGrayPhotometricCutDict instead."),
)
Definition at line 378 of file fgcmFitCycle.py.
◆ expVarGrayPhotometricCutDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on maximum exposure variance to be considered possibly "
"photometric. Must have one entry per band. Broad-band filters should be "
"0.0005."),
keytype=str,
itemtype=float,
default={},
)
Definition at line 386 of file fgcmFitCycle.py.
◆ filterMap
|
static |
Initial value:
= pexConfig.DictField(
doc="Mapping from 'filterName' to band.",
keytype=str,
itemtype=str,
default={},
)
Definition at line 99 of file fgcmFitCycle.py.
◆ fitBands
|
static |
Initial value:
= pexConfig.ListField(
doc=("Bands to use in atmospheric fit. The bands not listed here will have "
"the atmosphere constrained from the 'fitBands' on the same night. "
"Must be a subset of `config.bands`"),
dtype=str,
default=[],
)
Definition at line 76 of file fgcmFitCycle.py.
◆ fitFlag
|
static |
Initial value:
= pexConfig.ListField(
doc=("Flag for which bands are directly constrained in the FGCM fit. "
"Bands set to 0 will have the atmosphere constrained from observations "
"in other bands on the same night. Must be same length as config.bands, "
"and matched band-by-band."),
dtype=int,
default=(0,),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use fitBands instead."),
)
Definition at line 65 of file fgcmFitCycle.py.
◆ fitMirrorChromaticity
|
static |
Initial value:
= pexConfig.Field(
doc="Fit (intraband) mirror chromatic term?",
dtype=bool,
default=False,
)
Definition at line 569 of file fgcmFitCycle.py.
◆ focalPlaneSigmaClip
|
static |
Initial value:
= pexConfig.Field(
doc="Number of sigma to clip outliers per focal-plane.",
dtype=float,
default=4.0,
)
Definition at line 189 of file fgcmFitCycle.py.
◆ freezeStdAtmosphere
|
static |
Initial value:
= pexConfig.Field(
doc="Freeze atmosphere parameters to standard (for testing)",
dtype=bool,
default=False,
)
Definition at line 146 of file fgcmFitCycle.py.
◆ instrumentParsPerBand
|
static |
Initial value:
= pexConfig.Field(
doc=("Model instrumental parameters per band? "
"Otherwise, instrumental parameters (QE changes with time) are "
"shared among all bands."),
dtype=bool,
default=False,
)
Definition at line 556 of file fgcmFitCycle.py.
◆ instrumentSlopeMinDeltaT
|
static |
Initial value:
= pexConfig.Field(
doc=("Minimum time change (in days) between observations to use in constraining "
"instrument slope."),
dtype=float,
default=20.0,
)
Definition at line 563 of file fgcmFitCycle.py.
◆ isFinalCycle
|
static |
Initial value:
= pexConfig.Field(
doc=("Is this the final cycle of the fitting? Will automatically compute final "
"selection of stars and photometric exposures, and will output zeropoints "
"and standard stars for use in fgcmOutputProducts"),
dtype=bool,
default=False,
)
Definition at line 245 of file fgcmFitCycle.py.
◆ latitude
|
static |
Initial value:
= pexConfig.Field(
doc="Observatory latitude",
dtype=float,
default=None,
)
Definition at line 292 of file fgcmFitCycle.py.
◆ mapLongitudeRef
|
static |
Initial value:
= pexConfig.Field(
doc="Reference longitude for plotting maps",
dtype=float,
default=0.0,
)
Definition at line 512 of file fgcmFitCycle.py.
◆ mapNSide
|
static |
Initial value:
= pexConfig.Field(
doc="Healpix nside for plotting maps",
dtype=int,
default=256,
)
Definition at line 517 of file fgcmFitCycle.py.
◆ maxCcdGrayErr
|
static |
Initial value:
= pexConfig.Field(
doc="Maximum error on CCD gray offset to be considered photometric",
dtype=float,
default=0.05,
)
Definition at line 315 of file fgcmFitCycle.py.
◆ maxIterBeforeFinalCycle
|
static |
Initial value:
= pexConfig.Field(
doc=("Maximum fit iterations, prior to final cycle. The number of iterations "
"will always be 0 in the final cycle for cleanup and final selection."),
dtype=int,
default=50,
)
Definition at line 252 of file fgcmFitCycle.py.
◆ minCcdPerExp
|
static |
Initial value:
= pexConfig.Field(
doc=("Minimum number of good CCDs per exposure/visit to be used in calibration fit. "
"Visits with fewer good CCDs will have CCD zeropoints estimated where possible."),
dtype=int,
default=5,
)
Definition at line 309 of file fgcmFitCycle.py.
◆ minExpPerNight
|
static |
Initial value:
= pexConfig.Field(
doc="Minimum number of good exposures/visits to consider a partly photometric night",
dtype=int,
default=10,
)
Definition at line 326 of file fgcmFitCycle.py.
◆ minObsPerBand
|
static |
Initial value:
= pexConfig.Field(
doc="Minimum good observations per band",
dtype=int,
default=2,
)
Definition at line 285 of file fgcmFitCycle.py.
◆ minStarPerCcd
|
static |
Initial value:
= pexConfig.Field(
doc=("Minimum number of good stars per CCD to be used in calibration fit. "
"CCDs with fewer stars will have their calibration estimated from other "
"CCDs in the same visit, with zeropoint error increased accordingly."),
dtype=int,
default=5,
)
Definition at line 302 of file fgcmFitCycle.py.
◆ minStarPerExp
|
static |
Initial value:
= pexConfig.Field(
doc=("Minimum number of good stars per exposure/visit to be used in calibration fit. "
"Visits with fewer good stars will have CCD zeropoints estimated where possible."),
dtype=int,
default=600,
)
Definition at line 320 of file fgcmFitCycle.py.
◆ modelMagErrors
|
static |
Initial value:
= pexConfig.Field(
doc="Should FGCM model the magnitude errors from sky/fwhm? (False means trust inputs)",
dtype=bool,
default=True,
)
Definition at line 546 of file fgcmFitCycle.py.
◆ nCore
|
static |
Initial value:
= pexConfig.Field(
doc="Number of cores to use",
dtype=int,
default=4,
)
Definition at line 126 of file fgcmFitCycle.py.
◆ nExpPerRun
|
static |
Initial value:
= pexConfig.Field(
doc="Number of exposures to run in each chunk",
dtype=int,
default=1000,
)
Definition at line 136 of file fgcmFitCycle.py.
◆ nStarPerRun
|
static |
Initial value:
= pexConfig.Field(
doc="Number of stars to run in each chunk",
dtype=int,
default=200000,
)
Definition at line 131 of file fgcmFitCycle.py.
◆ outfileBase
|
static |
Initial value:
= pexConfig.Field(
doc="Filename start for plot output files",
dtype=str,
default=None,
)
Definition at line 522 of file fgcmFitCycle.py.
◆ outputStandardsBeforeFinalCycle
|
static |
Initial value:
= pexConfig.Field(
doc="Output standard stars prior to final cycle? Used in debugging.",
dtype=bool,
default=False,
)
Definition at line 579 of file fgcmFitCycle.py.
◆ outputZeropointsBeforeFinalCycle
|
static |
Initial value:
= pexConfig.Field(
doc="Output standard stars prior to final cycle? Used in debugging.",
dtype=bool,
default=False,
)
Definition at line 584 of file fgcmFitCycle.py.
◆ precomputeSuperStarInitialCycle
|
static |
Initial value:
= pexConfig.Field(
doc="Precompute superstar flat for initial cycle",
dtype=bool,
default=False,
)
Definition at line 151 of file fgcmFitCycle.py.
◆ quietMode
|
static |
Initial value:
= pexConfig.Field(
doc="Be less verbose with logging.",
dtype=bool,
default=False,
)
Definition at line 622 of file fgcmFitCycle.py.
◆ randomSeed
|
static |
Initial value:
= pexConfig.Field(
doc="Random seed for fgcm for consistency in tests.",
dtype=int,
default=None,
optional=True,
)
Definition at line 627 of file fgcmFitCycle.py.
◆ refStarOutlierNSig
|
static |
Initial value:
= pexConfig.Field(
doc=("Number of sigma compared to average mag for reference star to be considered an outlier. "
"Computed per-band, and if it is an outlier in any band it is rejected from fits."),
dtype=float,
default=4.0,
)
Definition at line 115 of file fgcmFitCycle.py.
◆ refStarSnMin
|
static |
Initial value:
= pexConfig.Field(
doc="Reference star signal-to-noise minimum to use in calibration. Set to <=0 for no cut.",
dtype=float,
default=50.0,
)
Definition at line 110 of file fgcmFitCycle.py.
◆ requiredBands
|
static |
Initial value:
= pexConfig.ListField(
doc=("Bands that are required for a star to be considered a calibration star. "
"Must be a subset of `config.bands`"),
dtype=str,
default=[],
)
Definition at line 93 of file fgcmFitCycle.py.
◆ requiredFlag
|
static |
Initial value:
= pexConfig.ListField(
doc=("Flag for which bands are required for a star to be considered a calibration "
"star in the FGCM fit. Typically this should be the same as fitFlag. Must "
"be same length as config.bands, and matched band-by-band."),
dtype=int,
default=(0,),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use requiredBands instead."),
)
Definition at line 83 of file fgcmFitCycle.py.
◆ reserveFraction
|
static |
Initial value:
= pexConfig.Field(
doc="Fraction of stars to reserve for testing",
dtype=float,
default=0.1,
)
Definition at line 141 of file fgcmFitCycle.py.
◆ sedboundaryterms
|
static |
Initial value:
= pexConfig.ConfigField(
doc="Mapping from bands to SED boundary term names used is sedterms.",
dtype=SedboundarytermDict,
)
Definition at line 439 of file fgcmFitCycle.py.
◆ sedFudgeFactors
|
static |
Initial value:
= pexConfig.ListField(
doc=("Fudge factors for computing linear SED from colors. Must be same length as "
"config.bands, and matched band-by-band."),
dtype=float,
default=(0,),
optional=True,
deprecated=("This field has been deprecated and will be removed after v20. "
"Please use sedSlopeTermMap and sedSlopeMap."),
)
Definition at line 430 of file fgcmFitCycle.py.
◆ sedterms
|
static |
Initial value:
= pexConfig.ConfigField(
doc="Mapping from terms to bands for fgcm linear SED approximations.",
dtype=SedtermDict,
)
Definition at line 443 of file fgcmFitCycle.py.
◆ sigFgcmMaxEGray
|
static |
Initial value:
= pexConfig.ListField(
doc=("Maximum (absolute) gray value for observation in sigma_FGCM. "
"May be 1 element (same for all bands) or the same length as config.bands."),
dtype=float,
default=(0.05,),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use sigFgcmMaxEGrayDict instead."),
)
Definition at line 452 of file fgcmFitCycle.py.
◆ sigFgcmMaxEGrayDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification for maximum (absolute) achromatic residual (gray value) "
"for observations in sigma_fgcm (raw repeatability). Broad-band filters "
"should be 0.05."),
keytype=str,
itemtype=float,
default={},
)
Definition at line 461 of file fgcmFitCycle.py.
◆ sigFgcmMaxErr
|
static |
Initial value:
= pexConfig.Field(
doc="Maximum mag error for fitting sigma_FGCM",
dtype=float,
default=0.01,
)
Definition at line 447 of file fgcmFitCycle.py.
◆ sigma0Phot
|
static |
Initial value:
= pexConfig.Field(
doc="Systematic error floor for all zeropoints",
dtype=float,
default=0.003,
)
Definition at line 507 of file fgcmFitCycle.py.
◆ sigmaCalFitPercentile
|
static |
Initial value:
= pexConfig.ListField(
doc="Magnitude percentile range to fit systematic error floor",
dtype=float,
default=(0.05, 0.15),
)
Definition at line 497 of file fgcmFitCycle.py.
◆ sigmaCalPlotPercentile
|
static |
Initial value:
= pexConfig.ListField(
doc="Magnitude percentile range to plot systematic error floor",
dtype=float,
default=(0.05, 0.95),
)
Definition at line 502 of file fgcmFitCycle.py.
◆ sigmaCalRange
|
static |
Initial value:
= pexConfig.ListField(
doc="Allowed range for systematic error floor estimation",
dtype=float,
default=(0.001, 0.003),
)
Definition at line 492 of file fgcmFitCycle.py.
◆ starColorCuts
|
static |
Initial value:
= pexConfig.ListField(
doc="Encoded star-color cuts (to be cleaned up)",
dtype=str,
default=("NO_DATA",),
)
Definition at line 527 of file fgcmFitCycle.py.
◆ superStarSigmaClip
|
static |
Initial value:
= pexConfig.Field(
doc="Number of sigma to clip outliers when selecting for superstar flats",
dtype=float,
default=5.0,
)
Definition at line 184 of file fgcmFitCycle.py.
◆ superStarSubCcd
|
static |
Initial value:
= pexConfig.Field(
doc="Compute superstar flat on sub-ccd scale",
dtype=bool,
default=True,
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use superStarSubCcdDict instead."),
)
Definition at line 156 of file fgcmFitCycle.py.
◆ superStarSubCcdChebyshevOrder
|
static |
Initial value:
= pexConfig.Field(
doc=("Order of the 2D chebyshev polynomials for sub-ccd superstar fit. "
"Global default is first-order polynomials, and should be overridden "
"on a camera-by-camera basis depending on the ISR."),
dtype=int,
default=1,
)
Definition at line 171 of file fgcmFitCycle.py.
◆ superStarSubCcdDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on whether to compute superstar flat on sub-ccd scale. "
"Must have one entry per band."),
keytype=str,
itemtype=bool,
default={},
)
Definition at line 164 of file fgcmFitCycle.py.
◆ superStarSubCcdTriangular
|
static |
Initial value:
= pexConfig.Field(
doc=("Should the sub-ccd superstar chebyshev matrix be triangular to "
"suppress high-order cross terms?"),
dtype=bool,
default=False,
)
Definition at line 178 of file fgcmFitCycle.py.
◆ useQuadraticPwv
|
static |
Initial value:
= pexConfig.Field(
doc="Model PWV with a quadratic term for variation through the night?",
dtype=bool,
default=False,
)
Definition at line 551 of file fgcmFitCycle.py.
◆ useRepeatabilityForExpGrayCuts
|
static |
Initial value:
= pexConfig.ListField(
doc=("Use star repeatability (instead of exposures) for computing photometric "
"cuts? Recommended for tract mode or bands with few exposures. "
"May be 1 element (same for all bands) or the same length as config.bands."),
dtype=bool,
default=(False,),
optional=True,
deprecated=("This field is no longer used, and has been deprecated by DM-23699. "
"It will be removed after v20. Use useRepeatabilityForExpGrayCutsDict instead."),
)
Definition at line 589 of file fgcmFitCycle.py.
◆ useRepeatabilityForExpGrayCutsDict
|
static |
Initial value:
= pexConfig.DictField(
doc=("Per-band specification on whether to use star repeatability (instead of exposures) "
"for computing photometric cuts. Recommended for tract mode or bands with few visits."),
keytype=str,
itemtype=bool,
default={},
)
Definition at line 599 of file fgcmFitCycle.py.
◆ utBoundary
|
static |
Initial value:
= pexConfig.Field(
doc="Boundary (in UTC) from day-to-day",
dtype=float,
default=None,
)
Definition at line 270 of file fgcmFitCycle.py.
◆ washMjds
|
static |
Initial value:
= pexConfig.ListField(
doc="Mirror wash MJDs",
dtype=float,
default=(0.0,),
)
Definition at line 275 of file fgcmFitCycle.py.
The documentation for this class was generated from the following file:
- /j/snowflake/release/lsstsw/stack/0.1.5/Linux64/fgcmcal/21.0.0-4-g8a80011+f67daf2f53/python/lsst/fgcmcal/fgcmFitCycle.py
