import lsst.fgcmcal.fgcmCalibrateTract assert type(config)==lsst.fgcmcal.fgcmCalibrateTract.FgcmCalibrateTractConfig, 'config is of type %s.%s instead of lsst.fgcmcal.fgcmCalibrateTract.FgcmCalibrateTractConfig' % (type(config).__module__, type(config).__name__) import lsst.fgcmcal.fgcmBuildStars import lsst.meas.algorithms.indexerRegistry import lsst.meas.astrom.directMatch import lsst.fgcmcal.sedterms import lsst.meas.algorithms.matcherSourceSelector import lsst.fgcmcal.fgcmLoadReferenceCatalog import lsst.meas.algorithms.astrometrySourceSelector import lsst.pipe.tasks.photoCal import lsst.meas.algorithms.objectSizeStarSelector import lsst.meas.algorithms.loadIndexedReferenceObjects import lsst.meas.algorithms.sourceSelector import lsst.fgcmcal.fgcmFitCycle import lsst.meas.algorithms.flaggedSourceSelector import lsst.meas.algorithms.ingestIndexReferenceTask import lsst.fgcmcal.fgcmOutputProducts import lsst.meas.algorithms.reserveSourcesTask import lsst.pipe.tasks.colorterms # Faull name of the source instFlux field to use, including 'instFlux'. The associated flag will be implicitly included in badFlags config.fgcmBuildStars.instFluxField='slot_CalibFlux_instFlux' # Minimum observations per band config.fgcmBuildStars.minPerBand=2 # Match radius (arcseconds) config.fgcmBuildStars.matchRadius=1.0 # Isolation radius (arcseconds) config.fgcmBuildStars.isolationRadius=2.0 # Density cut healpix nside config.fgcmBuildStars.densityCutNside=128 # Density cut number of stars per pixel config.fgcmBuildStars.densityCutMaxPerPixel=2000 # Healpix Nside for matching config.fgcmBuildStars.matchNside=4096 # Healpix coarse Nside for partitioning matches config.fgcmBuildStars.coarseNside=8 # Mapping from 'filterName' to band. config.fgcmBuildStars.filterMap={'g': 'g', 'r': 'r', 'r2': 'r', 'i': 'i', 'i2': 'i', 'z': 'z', 'y': 'y', 'N387': 'N387', 'N816': 'N816', 'N921': 'N921', 'N1010': 'N1010'} # Bands required for each star config.fgcmBuildStars.requiredBands=[] # Bands for 'primary' star matches. A star must be observed in one of these bands to be considered as a calibration star. config.fgcmBuildStars.primaryBands=['i', 'r', 'g', 'z', 'y', 'N387', 'N816', 'N921', 'N1010'] # dataRef name for the 'visit' field, usually 'visit'. config.fgcmBuildStars.visitDataRefName='visit' # dataRef name for the 'ccd' field, usually 'ccd' or 'detector'. config.fgcmBuildStars.ccdDataRefName='ccd' # Apply the jacobian of the WCS to the star observations prior to fit? config.fgcmBuildStars.doApplyWcsJacobian=True # Name of field with psf candidate flag for propagation config.fgcmBuildStars.psfCandidateName='calib_psf_candidate' # Subtract the local background before performing calibration? This is only supported for circular aperture calibration fluxes. config.fgcmBuildStars.doSubtractLocalBackground=True # Full name of the local background instFlux field to use. config.fgcmBuildStars.localBackgroundFluxField='base_LocalBackground_instFlux' # Apply flux limit? config.fgcmBuildStars.sourceSelector['science'].doFluxLimit=False # Apply flag limitation? config.fgcmBuildStars.sourceSelector['science'].doFlags=True # Apply unresolved limitation? config.fgcmBuildStars.sourceSelector['science'].doUnresolved=True # Apply signal-to-noise limit? config.fgcmBuildStars.sourceSelector['science'].doSignalToNoise=True # Apply isolated limitation? config.fgcmBuildStars.sourceSelector['science'].doIsolated=True # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['science'].fluxLimit.minimum=None # Select objects with value less than this config.fgcmBuildStars.sourceSelector['science'].fluxLimit.maximum=None # Name of the source flux field to use. config.fgcmBuildStars.sourceSelector['science'].fluxLimit.fluxField='slot_CalibFlux_instFlux' # List of source flag fields that must be set for a source to be used. config.fgcmBuildStars.sourceSelector['science'].flags.good=[] # List of source flag fields that must NOT be set for a source to be used. config.fgcmBuildStars.sourceSelector['science'].flags.bad=['base_PixelFlags_flag_edge', 'base_PixelFlags_flag_interpolatedCenter', 'base_PixelFlags_flag_saturatedCenter', 'base_PixelFlags_flag_crCenter', 'base_PixelFlags_flag_bad', 'base_PixelFlags_flag_interpolated', 'base_PixelFlags_flag_saturated', 'slot_Centroid_flag', 'slot_CalibFlux_flag'] # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['science'].unresolved.minimum=None # Select objects with value less than this config.fgcmBuildStars.sourceSelector['science'].unresolved.maximum=0.5 # Name of column for star/galaxy separation config.fgcmBuildStars.sourceSelector['science'].unresolved.name='base_ClassificationExtendedness_value' # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['science'].signalToNoise.minimum=10.0 # Select objects with value less than this config.fgcmBuildStars.sourceSelector['science'].signalToNoise.maximum=1000.0 # Name of the source flux field to use. config.fgcmBuildStars.sourceSelector['science'].signalToNoise.fluxField='slot_CalibFlux_instFlux' # Name of the source flux error field to use. config.fgcmBuildStars.sourceSelector['science'].signalToNoise.errField='slot_CalibFlux_instFluxErr' # Name of column for parent config.fgcmBuildStars.sourceSelector['science'].isolated.parentName='parent' # Name of column for nChild config.fgcmBuildStars.sourceSelector['science'].isolated.nChildName='deblend_nChild' # Apply magnitude limit? config.fgcmBuildStars.sourceSelector['references'].doMagLimit=False # Apply flag limitation? config.fgcmBuildStars.sourceSelector['references'].doFlags=False # Apply unresolved limitation? config.fgcmBuildStars.sourceSelector['references'].doUnresolved=False # Apply signal-to-noise limit? config.fgcmBuildStars.sourceSelector['references'].doSignalToNoise=False # Apply magnitude error limit? config.fgcmBuildStars.sourceSelector['references'].doMagError=False # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['references'].magLimit.minimum=None # Select objects with value less than this config.fgcmBuildStars.sourceSelector['references'].magLimit.maximum=None # Name of the source flux field to use. config.fgcmBuildStars.sourceSelector['references'].magLimit.fluxField='flux' # List of source flag fields that must be set for a source to be used. config.fgcmBuildStars.sourceSelector['references'].flags.good=[] # List of source flag fields that must NOT be set for a source to be used. config.fgcmBuildStars.sourceSelector['references'].flags.bad=[] # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['references'].unresolved.minimum=None # Select objects with value less than this config.fgcmBuildStars.sourceSelector['references'].unresolved.maximum=0.5 # Name of column for star/galaxy separation config.fgcmBuildStars.sourceSelector['references'].unresolved.name='base_ClassificationExtendedness_value' # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['references'].signalToNoise.minimum=None # Select objects with value less than this config.fgcmBuildStars.sourceSelector['references'].signalToNoise.maximum=None # Name of the source flux field to use. config.fgcmBuildStars.sourceSelector['references'].signalToNoise.fluxField='flux' # Name of the source flux error field to use. config.fgcmBuildStars.sourceSelector['references'].signalToNoise.errField='flux_err' # Select objects with value greater than this config.fgcmBuildStars.sourceSelector['references'].magError.minimum=None # Select objects with value less than this config.fgcmBuildStars.sourceSelector['references'].magError.maximum=None # Name of the source flux error field to use. config.fgcmBuildStars.sourceSelector['references'].magError.magErrField='mag_err' config.fgcmBuildStars.sourceSelector['references'].colorLimits={} # Apply flux limit to Psf Candidate selection? config.fgcmBuildStars.sourceSelector['objectSize'].doFluxLimit=True # specify the minimum psfFlux for good Psf Candidates config.fgcmBuildStars.sourceSelector['objectSize'].fluxMin=12500.0 # specify the maximum psfFlux for good Psf Candidates (ignored if == 0) config.fgcmBuildStars.sourceSelector['objectSize'].fluxMax=0.0 # Apply signal-to-noise (i.e. flux/fluxErr) limit to Psf Candidate selection? config.fgcmBuildStars.sourceSelector['objectSize'].doSignalToNoiseLimit=False # specify the minimum signal-to-noise for good Psf Candidates config.fgcmBuildStars.sourceSelector['objectSize'].signalToNoiseMin=20.0 # specify the maximum signal-to-noise for good Psf Candidates (ignored if == 0) config.fgcmBuildStars.sourceSelector['objectSize'].signalToNoiseMax=0.0 # minimum width to include in histogram config.fgcmBuildStars.sourceSelector['objectSize'].widthMin=0.0 # maximum width to include in histogram config.fgcmBuildStars.sourceSelector['objectSize'].widthMax=10.0 # Name of field in Source to use for flux measurement config.fgcmBuildStars.sourceSelector['objectSize'].sourceFluxField='base_GaussianFlux_instFlux' # Standard deviation of width allowed to be interpreted as good stars config.fgcmBuildStars.sourceSelector['objectSize'].widthStdAllowed=0.15 # Keep objects within this many sigma of cluster 0's median config.fgcmBuildStars.sourceSelector['objectSize'].nSigmaClip=2.0 # List of flags which cause a source to be rejected as bad config.fgcmBuildStars.sourceSelector['objectSize'].badFlags=['base_PixelFlags_flag_edge', 'base_PixelFlags_flag_interpolatedCenter', 'base_PixelFlags_flag_saturatedCenter', 'base_PixelFlags_flag_crCenter', 'base_PixelFlags_flag_bad', 'base_PixelFlags_flag_interpolated'] # Name of a flag field that is True for Sources that should be used. config.fgcmBuildStars.sourceSelector['flagged'].field='calib_psf_used' # List of flags which cause a source to be rejected as bad config.fgcmBuildStars.sourceSelector['astrometry'].badFlags=['base_PixelFlags_flag_edge', 'base_PixelFlags_flag_interpolatedCenter', 'base_PixelFlags_flag_saturatedCenter', 'base_PixelFlags_flag_crCenter', 'base_PixelFlags_flag_bad'] # Type of source flux; typically one of Ap or Psf config.fgcmBuildStars.sourceSelector['astrometry'].sourceFluxType='Ap' # Minimum allowed signal-to-noise ratio for sources used for matching (in the flux specified by sourceFluxType); <= 0 for no limit config.fgcmBuildStars.sourceSelector['astrometry'].minSnr=10.0 # Type of source flux; typically one of Ap or Psf config.fgcmBuildStars.sourceSelector['matcher'].sourceFluxType='Ap' # Minimum allowed signal-to-noise ratio for sources used for matching (in the flux specified by sourceFluxType); <= 0 for no limit config.fgcmBuildStars.sourceSelector['matcher'].minSnr=40.0 # Exclude objects that have saturated, interpolated, or edge pixels using PixelFlags. For matchOptimisticB set this to False to recover previous matcher selector behavior. config.fgcmBuildStars.sourceSelector['matcher'].excludePixelFlags=True config.fgcmBuildStars.sourceSelector.name='science' # Full name of instFlux field that contains inner aperture flux for aperture correction proxy config.fgcmBuildStars.apertureInnerInstFluxField='base_CircularApertureFlux_12_0_instFlux' # Full name of instFlux field that contains outer aperture flux for aperture correction proxy config.fgcmBuildStars.apertureOuterInstFluxField='base_CircularApertureFlux_17_0_instFlux' # Match reference catalog as additional constraint on calibration config.fgcmBuildStars.doReferenceMatches=True # Padding to add to 4 all edges of the bounding box (pixels) config.fgcmBuildStars.fgcmLoadReferenceCatalog.refObjLoader.pixelMargin=300 # Default reference catalog filter to use if filter not specified in exposure; if blank then filter must be specified in exposure. config.fgcmBuildStars.fgcmLoadReferenceCatalog.refObjLoader.defaultFilter='' # Always use this reference catalog filter, no matter whether or what filter name is supplied to the loader. Effectively a trivial filterMap: map all filter names to this filter. This can be set for purely-astrometric catalogs (e.g. Gaia DR2) where there is only one reasonable choice for every camera filter->refcat mapping, but not for refcats used for photometry, which need a filterMap and/or colorterms/transmission corrections. config.fgcmBuildStars.fgcmLoadReferenceCatalog.refObjLoader.anyFilterMapsToThis=None # Mapping of camera filter name: reference catalog filter name; each reference filter must exist in the refcat. Note that this does not perform any bandpass corrections: it is just a lookup. config.fgcmBuildStars.fgcmLoadReferenceCatalog.refObjLoader.filterMap={} # Require that the fields needed to correct proper motion (epoch, pm_ra and pm_dec) are present? config.fgcmBuildStars.fgcmLoadReferenceCatalog.refObjLoader.requireProperMotion=False # Name of the ingested reference dataset config.fgcmBuildStars.fgcmLoadReferenceCatalog.refObjLoader.ref_dataset_name='ps1_pv3_3pi_20170110' # Mapping from camera 'filterName' to reference filter name. config.fgcmBuildStars.fgcmLoadReferenceCatalog.refFilterMap={'g': 'g', 'r': 'r', 'r2': 'r', 'i': 'i', 'i2': 'i', 'z': 'z', 'y': 'y', 'N387': 'g', 'N816': 'i', 'N921': 'z', 'N1010': 'y'} # Apply photometric color terms to reference stars?Requires that colorterms be set to a ColorTermLibrary config.fgcmBuildStars.fgcmLoadReferenceCatalog.applyColorTerms=True config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data={} config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*']=lsst.pipe.tasks.colorterms.ColortermDict() config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data={} config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['g']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['g'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['g'].secondary='g' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['g'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['g'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['g'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['r']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['r'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['r'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['r'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['r'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['r'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['i']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['i'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['i'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['i'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['i'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['i'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['z']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['z'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['z'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['z'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['z'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['z'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['y']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['y'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['y'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['y'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['y'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['y'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-G']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-G'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-G'].secondary='g' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-G'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-G'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-G'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-R']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-R'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-R'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-R'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-R'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-R'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-I']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-I'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-I'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-I'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-I'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-I'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Z']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Z'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Z'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Z'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Z'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Z'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Y']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Y'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Y'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Y'].c0=0.0 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Y'].c1=0.0 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['hsc*'].data['HSC-Y'].c2=0.0 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*']=lsst.pipe.tasks.colorterms.ColortermDict() config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data={} config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['g']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['g'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['g'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['g'].c0=-0.009777 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['g'].c1=-0.077235 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['g'].c2=-0.013121 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r'].c0=-0.000711 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r'].c1=-0.006847 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r'].c2=-0.03511 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r2'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r2'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r2'].c0=-0.000632 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r2'].c1=-0.011237 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['r2'].c2=-0.038169 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i'].c0=0.000357 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i'].c1=-0.15329 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i'].c2=-0.009277 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i2'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i2'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i2'].c0=0.001278 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i2'].c1=-0.213569 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['i2'].c2=-0.012523 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['z']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['z'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['z'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['z'].c0=-0.005761 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['z'].c1=0.001317 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['z'].c2=-0.035334 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['y']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['y'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['y'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['y'].c0=0.003386 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['y'].c1=0.428877 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['y'].c2=0.076738 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['I945']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['I945'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['I945'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['I945'].c0=0.008117 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['I945'].c1=0.234991 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['I945'].c2=-0.042255 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N387']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N387'].primary='u' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N387'].secondary='g' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N387'].c0=-0.709229 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N387'].c1=0.310719 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N387'].c2=-0.044107 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N400']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N400'].primary='u' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N400'].secondary='g' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N400'].c0=-0.396264 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N400'].c1=-0.395133 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N400'].c2=0.038688 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N468']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N468'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N468'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N468'].c0=-0.059159 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N468'].c1=-0.030881 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N468'].c2=0.015356 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N515']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N515'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N515'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N515'].c0=-0.03251 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N515'].c1=-0.35444 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N515'].c2=0.100832 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N527']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N527'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N527'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N527'].c0=-0.0294 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N527'].c1=-0.453037 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N527'].c2=0.020922 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N656']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N656'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N656'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N656'].c0=0.037014 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N656'].c1=-0.538947 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N656'].c2=0.052489 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N718']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N718'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N718'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N718'].c0=-0.014742 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N718'].c1=-0.787571 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N718'].c2=0.237867 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N816']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N816'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N816'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N816'].c0=0.012676 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N816'].c1=-0.660317 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N816'].c2=0.055566 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N921']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N921'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N921'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N921'].c0=0.004619 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N921'].c1=0.093019 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N921'].c2=-0.126377 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N926']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N926'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N926'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N926'].c0=0.009369 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N926'].c1=0.130261 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N926'].c2=-0.119282 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N973']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N973'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N973'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N973'].c0=-0.005805 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N973'].c1=0.220412 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N973'].c2=-0.249072 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N1010']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N1010'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N1010'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N1010'].c0=0.015296 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N1010'].c1=0.794152 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['N1010'].c2=0.465309 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-G']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-G'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-G'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-G'].c0=-0.009777 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-G'].c1=-0.077235 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-G'].c2=-0.013121 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R'].c0=-0.000711 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R'].c1=-0.006847 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R'].c2=-0.03511 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R2'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R2'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R2'].c0=-0.000632 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R2'].c1=-0.011237 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-R2'].c2=-0.038169 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I'].c0=0.000357 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I'].c1=-0.15329 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I'].c2=-0.009277 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I2'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I2'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I2'].c0=0.001278 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I2'].c1=-0.213569 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-I2'].c2=-0.012523 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-Z']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-Z'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-Z'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-Z'].c0=-0.005761 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-Z'].c1=0.001317 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-Z'].c2=-0.035334 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-y']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-y'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-y'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-y'].c0=0.003386 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-y'].c1=0.428877 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['HSC-y'].c2=0.076738 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['IB0945']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['IB0945'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['IB0945'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['IB0945'].c0=0.008117 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['IB0945'].c1=0.234991 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['IB0945'].c2=-0.042255 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0387']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0387'].primary='u' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0387'].secondary='g' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0387'].c0=-0.709229 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0387'].c1=0.310719 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0387'].c2=-0.044107 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0400']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0400'].primary='u' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0400'].secondary='g' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0400'].c0=-0.396264 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0400'].c1=-0.395133 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0400'].c2=0.038688 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0468']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0468'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0468'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0468'].c0=-0.059159 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0468'].c1=-0.030881 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0468'].c2=0.015356 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0515']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0515'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0515'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0515'].c0=-0.03251 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0515'].c1=-0.35444 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0515'].c2=0.100832 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0527']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0527'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0527'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0527'].c0=-0.0294 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0527'].c1=-0.453037 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0527'].c2=0.020922 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0656']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0656'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0656'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0656'].c0=0.037014 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0656'].c1=-0.538947 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0656'].c2=0.052489 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0718']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0718'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0718'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0718'].c0=-0.014742 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0718'].c1=-0.787571 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0718'].c2=0.237867 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0816']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0816'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0816'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0816'].c0=0.012676 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0816'].c1=-0.660317 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0816'].c2=0.055566 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0921']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0921'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0921'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0921'].c0=0.004619 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0921'].c1=0.093019 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0921'].c2=-0.126377 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0926']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0926'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0926'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0926'].c0=0.009369 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0926'].c1=0.130261 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0926'].c2=-0.119282 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0973']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0973'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0973'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0973'].c0=-0.005805 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0973'].c1=0.220412 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB0973'].c2=-0.249072 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB01010']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB01010'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB01010'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB01010'].c0=0.015296 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB01010'].c1=0.794152 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['sdss*'].data['NB01010'].c2=0.465309 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*']=lsst.pipe.tasks.colorterms.ColortermDict() config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data={} config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['g']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['g'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['g'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['g'].c0=0.005728 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['g'].c1=0.061749 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['g'].c2=-0.001125 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r'].c0=-0.000144 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r'].c1=0.001369 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r'].c2=-0.00838 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r2'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r2'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r2'].c0=-3.2e-05 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r2'].c1=-0.002866 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['r2'].c2=-0.012638 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i'].c0=0.000643 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i'].c1=-0.130078 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i'].c2=-0.006855 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i2'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i2'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i2'].c0=0.001625 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i2'].c1=-0.200406 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['i2'].c2=-0.013666 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['z']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['z'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['z'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['z'].c0=-0.005362 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['z'].c1=-0.221551 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['z'].c2=-0.308279 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['y']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['y'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['y'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['y'].c0=-0.002055 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['y'].c1=0.20968 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['y'].c2=0.227296 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['I945']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['I945'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['I945'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['I945'].c0=0.005275 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['I945'].c1=-0.194285 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['I945'].c2=-0.125424 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N387']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N387'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N387'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N387'].c0=0.427879 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N387'].c1=1.869068 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N387'].c2=0.54058 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N400']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N400'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N400'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N400'].c0=0.176542 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N400'].c1=1.127055 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N400'].c2=0.505502 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N468']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N468'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N468'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N468'].c0=-0.04224 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N468'].c1=0.121756 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N468'].c2=0.027599 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N515']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N515'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N515'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N515'].c0=-0.021913 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N515'].c1=-0.253159 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N515'].c2=0.151553 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N527']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N527'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N527'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N527'].c0=-0.020641 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N527'].c1=-0.366167 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N527'].c2=0.038497 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N656']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N656'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N656'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N656'].c0=0.035655 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N656'].c1=-0.512046 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N656'].c2=0.042796 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N718']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N718'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N718'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N718'].c0=-0.016294 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N718'].c1=-0.233139 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N718'].c2=0.252505 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N816']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N816'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N816'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N816'].c0=0.013806 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N816'].c1=-0.717681 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N816'].c2=0.049289 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N921']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N921'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N921'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N921'].c0=0.002039 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N921'].c1=-0.477412 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N921'].c2=-0.492151 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N926']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N926'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N926'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N926'].c0=0.00523 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N926'].c1=-0.574448 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N926'].c2=-0.330899 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N973']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N973'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N973'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N973'].c0=-0.007775 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N973'].c1=-0.050972 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N973'].c2=-0.197278 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N1010']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N1010'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N1010'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N1010'].c0=0.003607 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N1010'].c1=0.865366 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['N1010'].c2=1.271817 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-G']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-G'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-G'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-G'].c0=0.005728 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-G'].c1=0.061749 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-G'].c2=-0.001125 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R'].c0=-0.000144 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R'].c1=0.001369 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R'].c2=-0.00838 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R2'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R2'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R2'].c0=-3.2e-05 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R2'].c1=-0.002866 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-R2'].c2=-0.012638 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I'].c0=0.000643 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I'].c1=-0.130078 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I'].c2=-0.006855 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I2']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I2'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I2'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I2'].c0=0.001625 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I2'].c1=-0.200406 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-I2'].c2=-0.013666 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Z']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Z'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Z'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Z'].c0=-0.005362 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Z'].c1=-0.221551 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Z'].c2=-0.308279 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Y']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Y'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Y'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Y'].c0=-0.002055 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Y'].c1=0.20968 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['HSC-Y'].c2=0.227296 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['IB0945']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['IB0945'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['IB0945'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['IB0945'].c0=0.005275 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['IB0945'].c1=-0.194285 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['IB0945'].c2=-0.125424 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0387']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0387'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0387'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0387'].c0=0.427879 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0387'].c1=1.869068 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0387'].c2=0.54058 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0400']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0400'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0400'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0400'].c0=0.176542 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0400'].c1=1.127055 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0400'].c2=0.505502 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0468']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0468'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0468'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0468'].c0=-0.04224 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0468'].c1=0.121756 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0468'].c2=0.027599 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0515']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0515'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0515'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0515'].c0=-0.021913 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0515'].c1=-0.253159 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0515'].c2=0.151553 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0527']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0527'].primary='g' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0527'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0527'].c0=-0.020641 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0527'].c1=-0.366167 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0527'].c2=0.038497 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0656']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0656'].primary='r' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0656'].secondary='i' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0656'].c0=0.035655 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0656'].c1=-0.512046 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0656'].c2=0.042796 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0718']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0718'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0718'].secondary='r' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0718'].c0=-0.016294 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0718'].c1=-0.233139 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0718'].c2=0.252505 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0816']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0816'].primary='i' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0816'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0816'].c0=0.013806 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0816'].c1=-0.717681 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0816'].c2=0.049289 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0921']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0921'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0921'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0921'].c0=0.002039 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0921'].c1=-0.477412 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0921'].c2=-0.492151 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0926']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0926'].primary='z' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0926'].secondary='y' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0926'].c0=0.00523 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0926'].c1=-0.574448 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0926'].c2=-0.330899 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0973']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0973'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0973'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0973'].c0=-0.007775 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0973'].c1=-0.050972 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB0973'].c2=-0.197278 config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB01010']=lsst.pipe.tasks.colorterms.Colorterm() # name of primary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB01010'].primary='y' # name of secondary filter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB01010'].secondary='z' # Constant parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB01010'].c0=0.003607 # First-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB01010'].c1=0.865366 # Second-order parameter config.fgcmBuildStars.fgcmLoadReferenceCatalog.colorterms.data['ps1*'].data['NB01010'].c2=1.271817 # Apply magnitude limit? config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.doMagLimit=False # Apply flag limitation? config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.doFlags=False # Apply unresolved limitation? config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.doUnresolved=False # Apply signal-to-noise limit? config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.doSignalToNoise=True # Apply magnitude error limit? config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.doMagError=False # Select objects with value greater than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.magLimit.minimum=None # Select objects with value less than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.magLimit.maximum=None # Name of the source flux field to use. config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.magLimit.fluxField='flux' # List of source flag fields that must be set for a source to be used. config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.flags.good=[] # List of source flag fields that must NOT be set for a source to be used. config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.flags.bad=[] # Select objects with value greater than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.unresolved.minimum=None # Select objects with value less than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.unresolved.maximum=0.5 # Name of column for star/galaxy separation config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.unresolved.name='base_ClassificationExtendedness_value' # Select objects with value greater than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.signalToNoise.minimum=10.0 # Select objects with value less than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.signalToNoise.maximum=None # Name of the source flux field to use. config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.signalToNoise.fluxField='i_flux' # Name of the source flux error field to use. config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.signalToNoise.errField='i_fluxErr' # Select objects with value greater than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.magError.minimum=None # Select objects with value less than this config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.magError.maximum=None # Name of the source flux error field to use. config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.magError.magErrField='mag_err' config.fgcmBuildStars.fgcmLoadReferenceCatalog.referenceSelector.colorLimits={} # Number of visits read between checkpoints config.fgcmBuildStars.nVisitsPerCheckpoint=500 # Reference CCD for scanning visits config.fgcmBuildStars.referenceCCD=13 # Check repo for all CCDs for each visit specified. To be used when the full set of ids (visit/ccd) are not specified on the command line. For Gen2, specifying one ccd and setting checkAllCcds=True is significantly faster than the alternatives. config.fgcmBuildStars.checkAllCcds=False # Bands to run calibration config.fgcmFitCycle.bands=['N387', 'g', 'r', 'i', 'N816', 'z', 'N921', 'y', 'N1010'] # 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` config.fgcmFitCycle.fitBands=['N387', 'g', 'r', 'i', 'N816', 'z', 'N921', 'y', 'N1010'] # Bands that are required for a star to be considered a calibration star. Must be a subset of `config.bands` config.fgcmFitCycle.requiredBands=[] # Mapping from 'filterName' to band. config.fgcmFitCycle.filterMap={'g': 'g', 'r': 'r', 'r2': 'r', 'i': 'i', 'i2': 'i', 'z': 'z', 'y': 'y', 'N387': 'N387', 'N816': 'N816', 'N921': 'N921', 'N1010': 'N1010'} # Use reference catalog as additional constraint on calibration config.fgcmFitCycle.doReferenceCalibration=True # Reference star signal-to-noise minimum to use in calibration. Set to <=0 for no cut. config.fgcmFitCycle.refStarSnMin=50.0 # 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. config.fgcmFitCycle.refStarOutlierNSig=4.0 # Apply color cuts to reference stars? config.fgcmFitCycle.applyRefStarColorCuts=True # Number of cores to use config.fgcmFitCycle.nCore=4 # Number of stars to run in each chunk config.fgcmFitCycle.nStarPerRun=200000 # Number of exposures to run in each chunk config.fgcmFitCycle.nExpPerRun=1000 # Fraction of stars to reserve for testing config.fgcmFitCycle.reserveFraction=0.1 # Freeze atmosphere parameters to standard (for testing) config.fgcmFitCycle.freezeStdAtmosphere=True # Precompute superstar flat for initial cycle config.fgcmFitCycle.precomputeSuperStarInitialCycle=True # Per-band specification on whether to compute superstar flat on sub-ccd scale. Must have one entry per band. config.fgcmFitCycle.superStarSubCcdDict={'N387': False, 'g': True, 'r': True, 'i': True, 'N816': True, 'z': True, 'N921': True, 'y': True, 'N1010': False} # 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. config.fgcmFitCycle.superStarSubCcdChebyshevOrder=2 # Should the sub-ccd superstar chebyshev matrix be triangular to suppress high-order cross terms? config.fgcmFitCycle.superStarSubCcdTriangular=False # Number of sigma to clip outliers when selecting for superstar flats config.fgcmFitCycle.superStarSigmaClip=5.0 # Number of sigma to clip outliers per focal-plane. config.fgcmFitCycle.focalPlaneSigmaClip=4.0 # Per-band specification on whether to compute achromatic per-ccd residual ('ccd gray') on a sub-ccd scale. config.fgcmFitCycle.ccdGraySubCcdDict={'N387': False, 'g': True, 'r': True, 'i': True, 'N816': True, 'z': True, 'N921': True, 'y': True, 'N1010': False} # Order of the 2D chebyshev polynomials for sub-ccd gray fit. config.fgcmFitCycle.ccdGraySubCcdChebyshevOrder=1 # Should the sub-ccd gray chebyshev matrix be triangular to suppress high-order cross terms? config.fgcmFitCycle.ccdGraySubCcdTriangular=True # Per-band specification on whether to compute focal-plane residual ('ccd gray') corrections. config.fgcmFitCycle.ccdGrayFocalPlaneDict={'N387': True, 'g': True, 'r': True, 'i': True, 'N816': True, 'z': True, 'N921': True, 'y': True, 'N1010': True} # 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. config.fgcmFitCycle.ccdGrayFocalPlaneFitMinCcd=50 # Order of the 2D chebyshev polynomials for focal plane fit. config.fgcmFitCycle.ccdGrayFocalPlaneChebyshevOrder=3 # FGCM fit cycle number. This is automatically incremented after each run and stage of outlier rejection. See cookbook for details. config.fgcmFitCycle.cycleNumber=0 # 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 config.fgcmFitCycle.isFinalCycle=False # Maximum fit iterations, prior to final cycle. The number of iterations will always be 0 in the final cycle for cleanup and final selection. config.fgcmFitCycle.maxIterBeforeFinalCycle=75 # Percentile brightest stars on a visit/ccd to use to compute net offset from local background subtraction. config.fgcmFitCycle.deltaMagBkgOffsetPercentile=0.25 # Compute net offset from local background subtraction per-ccd? Otherwise, use computation per visit. config.fgcmFitCycle.deltaMagBkgPerCcd=False # Boundary (in UTC) from day-to-day config.fgcmFitCycle.utBoundary=0.0 # Mirror wash MJDs config.fgcmFitCycle.washMjds=[56650.0, 57500.0, 57700.0, 58050.0] # Epoch boundaries in MJD config.fgcmFitCycle.epochMjds=[56650.0, 57420.0, 57606.0, 59000.0] # Minimum good observations per band config.fgcmFitCycle.minObsPerBand=2 # Observatory latitude config.fgcmFitCycle.latitude=19.8256 # Maximum gray extinction to be considered bright observation config.fgcmFitCycle.brightObsGrayMax=0.15 # 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. config.fgcmFitCycle.minStarPerCcd=5 # 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. config.fgcmFitCycle.minCcdPerExp=5 # Maximum error on CCD gray offset to be considered photometric config.fgcmFitCycle.maxCcdGrayErr=0.05 # 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. config.fgcmFitCycle.minStarPerExp=100 # Minimum number of good exposures/visits to consider a partly photometric night config.fgcmFitCycle.minExpPerNight=3 # Maximum exposure/visit gray value for initial selection of possible photometric observations. config.fgcmFitCycle.expGrayInitialCut=-0.25 # 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. config.fgcmFitCycle.expGrayPhotometricCutDict={'N387': -0.05, 'g': -0.05, 'r': -0.05, 'i': -0.05, 'N816': -0.05, 'z': -0.05, 'N921': -0.05, 'y': -0.05, 'N1010': -0.05} # 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. config.fgcmFitCycle.expGrayHighCutDict={'N387': 0.2, 'g': 0.2, 'r': 0.2, 'i': 0.2, 'N816': 0.2, 'z': 0.2, 'N921': 0.2, 'y': 0.2, 'N1010': 0.2} # 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. config.fgcmFitCycle.expGrayRecoverCut=-1.0 # 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. config.fgcmFitCycle.expVarGrayPhotometricCutDict={'N387': 0.05, 'g': 0.0025, 'r': 0.0025, 'i': 0.0025, 'N816': 0.05, 'z': 0.0025, 'N921': 0.05, 'y': 0.0025, 'N1010': 0.05} # 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. config.fgcmFitCycle.expGrayErrRecoverCut=0.05 # Number of aperture bins used in aperture correction fit. When set to 0no fit will be performed, and the config.aperCorrInputSlopes will be used if available. config.fgcmFitCycle.aperCorrFitNBins=0 # 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). config.fgcmFitCycle.aperCorrInputSlopeDict={'N387': -1.0, 'g': -1.1579, 'r': -1.3908, 'i': -1.1436, 'N816': -1.8149, 'z': -1.6974, 'N921': -1.331, 'y': -1.2057, 'N1010': -1.0} config.fgcmFitCycle.sedboundaryterms.data={} config.fgcmFitCycle.sedboundaryterms.data['gr']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['gr'].primary='g' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['gr'].secondary='r' config.fgcmFitCycle.sedboundaryterms.data['ri']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['ri'].primary='r' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['ri'].secondary='i' config.fgcmFitCycle.sedboundaryterms.data['iz']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['iz'].primary='i' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['iz'].secondary='z' config.fgcmFitCycle.sedboundaryterms.data['zy']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['zy'].primary='z' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['zy'].secondary='y' config.fgcmFitCycle.sedboundaryterms.data['N387g']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['N387g'].primary='N387' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['N387g'].secondary='g' config.fgcmFitCycle.sedboundaryterms.data['N816i']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['N816i'].primary='N816' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['N816i'].secondary='i' config.fgcmFitCycle.sedboundaryterms.data['N921z']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['N921z'].primary='N921' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['N921z'].secondary='z' config.fgcmFitCycle.sedboundaryterms.data['N1010y']=lsst.fgcmcal.sedterms.Sedboundaryterm() # name of primary band config.fgcmFitCycle.sedboundaryterms.data['N1010y'].primary='N1010' # name of secondary band config.fgcmFitCycle.sedboundaryterms.data['N1010y'].secondary='y' config.fgcmFitCycle.sedterms.data={} config.fgcmFitCycle.sedterms.data['g']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['g'].primaryTerm='gr' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['g'].secondaryTerm='ri' # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['g'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['g'].constant=1.6 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['g'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['g'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['g'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['r']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['r'].primaryTerm='gr' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['r'].secondaryTerm='ri' # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['r'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['r'].constant=0.9 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['r'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['r'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['r'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['i']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['i'].primaryTerm='ri' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['i'].secondaryTerm='iz' # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['i'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['i'].constant=1.0 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['i'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['i'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['i'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['z']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['z'].primaryTerm='iz' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['z'].secondaryTerm='zy' # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['z'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['z'].constant=1.0 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['z'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['z'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['z'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['y']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['y'].primaryTerm='zy' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['y'].secondaryTerm='iz' # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['y'].extrapolated=True # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['y'].constant=0.25 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['y'].primaryBand='y' # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['y'].secondaryBand='z' # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['y'].tertiaryBand='i' config.fgcmFitCycle.sedterms.data['N387']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N387'].primaryTerm='N387g' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N387'].secondaryTerm=None # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['N387'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['N387'].constant=1.0 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['N387'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['N387'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['N387'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['N816']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N816'].primaryTerm='N816i' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N816'].secondaryTerm=None # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['N816'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['N816'].constant=0.7 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['N816'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['N816'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['N816'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['N921']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N921'].primaryTerm='N921z' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N921'].secondaryTerm=None # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['N921'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['N921'].constant=0.5 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['N921'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['N921'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['N921'].tertiaryBand=None config.fgcmFitCycle.sedterms.data['N1010']=lsst.fgcmcal.sedterms.Sedterm() # Name of primary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N1010'].primaryTerm='N1010y' # Name of secondary Sedboundaryterm config.fgcmFitCycle.sedterms.data['N1010'].secondaryTerm=None # Extrapolate to compute SED slope config.fgcmFitCycle.sedterms.data['N1010'].extrapolated=False # Adjustment constant for SED slope config.fgcmFitCycle.sedterms.data['N1010'].constant=1.0 # Primary band name for extrapolation config.fgcmFitCycle.sedterms.data['N1010'].primaryBand=None # Secondary band name for extrapolation config.fgcmFitCycle.sedterms.data['N1010'].secondaryBand=None # Tertiary band name for extrapolation config.fgcmFitCycle.sedterms.data['N1010'].tertiaryBand=None # Maximum mag error for fitting sigma_FGCM config.fgcmFitCycle.sigFgcmMaxErr=0.01 # Per-band specification for maximum (absolute) achromatic residual (gray value) for observations in sigma_fgcm (raw repeatability). Broad-band filters should be 0.05. config.fgcmFitCycle.sigFgcmMaxEGrayDict={'N387': 0.15, 'g': 0.05, 'r': 0.05, 'i': 0.05, 'N816': 0.15, 'z': 0.05, 'N921': 0.15, 'y': 0.05, 'N1010': 0.15} # Maximum error on a star observation to use in ccd gray (achromatic residual) computation config.fgcmFitCycle.ccdGrayMaxStarErr=0.1 # 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. config.fgcmFitCycle.approxThroughputDict={'N387': 1.0, 'g': 1.0, 'r': 1.0, 'i': 1.0, 'N816': 1.0, 'z': 1.0, 'N921': 1.0, 'y': 1.0, 'N1010': 1.0} # Allowed range for systematic error floor estimation config.fgcmFitCycle.sigmaCalRange=[0.001, 0.003] # Magnitude percentile range to fit systematic error floor config.fgcmFitCycle.sigmaCalFitPercentile=[0.05, 0.15] # Magnitude percentile range to plot systematic error floor config.fgcmFitCycle.sigmaCalPlotPercentile=[0.05, 0.95] # Systematic error floor for all zeropoints config.fgcmFitCycle.sigma0Phot=0.003 # Reference longitude for plotting maps config.fgcmFitCycle.mapLongitudeRef=0.0 # Healpix nside for plotting maps config.fgcmFitCycle.mapNSide=256 # Filename start for plot output files config.fgcmFitCycle.outfileBase='fgcmHscCalibrations' # Encoded star-color cuts (to be cleaned up) config.fgcmFitCycle.starColorCuts=['g,r,-0.25,2.25', 'r,i,-0.50,2.25', 'i,z,-0.50,1.00', 'g,i,0.0,3.5'] # Band names to use to split stars by color. Must have 2 entries. config.fgcmFitCycle.colorSplitBands=['g', 'i'] # Should FGCM model the magnitude errors from sky/fwhm? (False means trust inputs) config.fgcmFitCycle.modelMagErrors=True # Model PWV with a quadratic term for variation through the night? config.fgcmFitCycle.useQuadraticPwv=False # Model instrumental parameters per band? Otherwise, instrumental parameters (QE changes with time) are shared among all bands. config.fgcmFitCycle.instrumentParsPerBand=True # Minimum time change (in days) between observations to use in constraining instrument slope. config.fgcmFitCycle.instrumentSlopeMinDeltaT=20.0 # Fit (intraband) mirror chromatic term? config.fgcmFitCycle.fitMirrorChromaticity=False # Mirror coating dates in MJD config.fgcmFitCycle.coatingMjds=[56650.0, 58050.0] # Output standard stars prior to final cycle? Used in debugging. config.fgcmFitCycle.outputStandardsBeforeFinalCycle=False # Output standard stars prior to final cycle? Used in debugging. config.fgcmFitCycle.outputZeropointsBeforeFinalCycle=False # 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. config.fgcmFitCycle.useRepeatabilityForExpGrayCutsDict={'N387': True, 'g': True, 'r': True, 'i': True, 'N816': True, 'z': True, 'N921': True, 'y': True, 'N1010': True} # 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). config.fgcmFitCycle.autoPhotometricCutNSig=3.0 # 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). config.fgcmFitCycle.autoHighCutNSig=4.0 # Be less verbose with logging. config.fgcmFitCycle.quietMode=True # Random seed for fgcm for consistency in tests. config.fgcmFitCycle.randomSeed=None # Final fit cycle from FGCM fit config.fgcmOutputProducts.cycleNumber=5 # Transfer 'absolute' calibration from reference catalog? This afterburner step is unnecessary if reference stars were used in the full fit in FgcmFitCycleTask. config.fgcmOutputProducts.doReferenceCalibration=False # Output standard stars in reference catalog format config.fgcmOutputProducts.doRefcatOutput=False # Output atmospheres in transmission_atmosphere_fgcm format config.fgcmOutputProducts.doAtmosphereOutput=True # Output zeropoints in fgcm_photoCalib format config.fgcmOutputProducts.doZeropointOutput=True # Compose Jacobian of WCS with fgcm calibration for output photoCalib? config.fgcmOutputProducts.doComposeWcsJacobian=True # Apply the mean chromatic correction to the zeropoints? config.fgcmOutputProducts.doApplyMeanChromaticCorrection=True # Padding to add to 4 all edges of the bounding box (pixels) config.fgcmOutputProducts.refObjLoader.pixelMargin=300 # Default reference catalog filter to use if filter not specified in exposure; if blank then filter must be specified in exposure. config.fgcmOutputProducts.refObjLoader.defaultFilter='' # Always use this reference catalog filter, no matter whether or what filter name is supplied to the loader. Effectively a trivial filterMap: map all filter names to this filter. This can be set for purely-astrometric catalogs (e.g. Gaia DR2) where there is only one reasonable choice for every camera filter->refcat mapping, but not for refcats used for photometry, which need a filterMap and/or colorterms/transmission corrections. config.fgcmOutputProducts.refObjLoader.anyFilterMapsToThis=None # Mapping of camera filter name: reference catalog filter name; each reference filter must exist in the refcat. Note that this does not perform any bandpass corrections: it is just a lookup. config.fgcmOutputProducts.refObjLoader.filterMap={} # Require that the fields needed to correct proper motion (epoch, pm_ra and pm_dec) are present? config.fgcmOutputProducts.refObjLoader.requireProperMotion=False # Name of the ingested reference dataset config.fgcmOutputProducts.refObjLoader.ref_dataset_name='cal_ref_cat' # Matching radius, arcsec config.fgcmOutputProducts.photoCal.match.matchRadius=0.25 # Apply flux limit? config.fgcmOutputProducts.photoCal.match.sourceSelection.doFluxLimit=False # Apply flag limitation? config.fgcmOutputProducts.photoCal.match.sourceSelection.doFlags=True # Apply unresolved limitation? config.fgcmOutputProducts.photoCal.match.sourceSelection.doUnresolved=False # Apply signal-to-noise limit? config.fgcmOutputProducts.photoCal.match.sourceSelection.doSignalToNoise=True # Apply isolated limitation? config.fgcmOutputProducts.photoCal.match.sourceSelection.doIsolated=False # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.sourceSelection.fluxLimit.minimum=None # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.sourceSelection.fluxLimit.maximum=None # Name of the source flux field to use. config.fgcmOutputProducts.photoCal.match.sourceSelection.fluxLimit.fluxField='slot_CalibFlux_instFlux' # List of source flag fields that must be set for a source to be used. config.fgcmOutputProducts.photoCal.match.sourceSelection.flags.good=[] # List of source flag fields that must NOT be set for a source to be used. config.fgcmOutputProducts.photoCal.match.sourceSelection.flags.bad=['flag_badStar'] # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.sourceSelection.unresolved.minimum=None # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.sourceSelection.unresolved.maximum=0.5 # Name of column for star/galaxy separation config.fgcmOutputProducts.photoCal.match.sourceSelection.unresolved.name='base_ClassificationExtendedness_value' # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.sourceSelection.signalToNoise.minimum=10.0 # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.sourceSelection.signalToNoise.maximum=None # Name of the source flux field to use. config.fgcmOutputProducts.photoCal.match.sourceSelection.signalToNoise.fluxField='instFlux' # Name of the source flux error field to use. config.fgcmOutputProducts.photoCal.match.sourceSelection.signalToNoise.errField='instFluxErr' # Name of column for parent config.fgcmOutputProducts.photoCal.match.sourceSelection.isolated.parentName='parent' # Name of column for nChild config.fgcmOutputProducts.photoCal.match.sourceSelection.isolated.nChildName='deblend_nChild' # Apply magnitude limit? config.fgcmOutputProducts.photoCal.match.referenceSelection.doMagLimit=False # Apply flag limitation? config.fgcmOutputProducts.photoCal.match.referenceSelection.doFlags=False # Apply unresolved limitation? config.fgcmOutputProducts.photoCal.match.referenceSelection.doUnresolved=False # Apply signal-to-noise limit? config.fgcmOutputProducts.photoCal.match.referenceSelection.doSignalToNoise=True # Apply magnitude error limit? config.fgcmOutputProducts.photoCal.match.referenceSelection.doMagError=False # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.referenceSelection.magLimit.minimum=None # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.referenceSelection.magLimit.maximum=None # Name of the source flux field to use. config.fgcmOutputProducts.photoCal.match.referenceSelection.magLimit.fluxField='flux' # List of source flag fields that must be set for a source to be used. config.fgcmOutputProducts.photoCal.match.referenceSelection.flags.good=[] # List of source flag fields that must NOT be set for a source to be used. config.fgcmOutputProducts.photoCal.match.referenceSelection.flags.bad=[] # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.referenceSelection.unresolved.minimum=None # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.referenceSelection.unresolved.maximum=0.5 # Name of column for star/galaxy separation config.fgcmOutputProducts.photoCal.match.referenceSelection.unresolved.name='base_ClassificationExtendedness_value' # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.referenceSelection.signalToNoise.minimum=10.0 # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.referenceSelection.signalToNoise.maximum=None # Name of the source flux field to use. config.fgcmOutputProducts.photoCal.match.referenceSelection.signalToNoise.fluxField='flux' # Name of the source flux error field to use. config.fgcmOutputProducts.photoCal.match.referenceSelection.signalToNoise.errField='flux_err' # Select objects with value greater than this config.fgcmOutputProducts.photoCal.match.referenceSelection.magError.minimum=None # Select objects with value less than this config.fgcmOutputProducts.photoCal.match.referenceSelection.magError.maximum=None # Name of the source flux error field to use. config.fgcmOutputProducts.photoCal.match.referenceSelection.magError.magErrField='mag_err' config.fgcmOutputProducts.photoCal.match.referenceSelection.colorLimits={} # Fraction of candidates to reserve from fitting; none if <= 0 config.fgcmOutputProducts.photoCal.reserve.fraction=0.0 # This number will be added to the exposure ID to set the random seed for reserving candidates config.fgcmOutputProducts.photoCal.reserve.seed=1 # Name of the source instFlux field to use. The associated flag field # ('_flags') will be implicitly included in badFlags. config.fgcmOutputProducts.photoCal.fluxField='instFlux' # Apply photometric color terms to reference stars? One of: # None: apply if colorterms and photoCatName are not None; # fail if color term data is not available for the specified ref catalog and filter. # True: always apply colorterms; fail if color term data is not available for the # specified reference catalog and filter. # False: do not apply. config.fgcmOutputProducts.photoCal.applyColorTerms=False # maximum sigma to use when clipping config.fgcmOutputProducts.photoCal.sigmaMax=0.25 # clip at nSigma config.fgcmOutputProducts.photoCal.nSigma=3.0 # use median instead of mean to compute zeropoint config.fgcmOutputProducts.photoCal.useMedian=True # number of iterations config.fgcmOutputProducts.photoCal.nIter=20 config.fgcmOutputProducts.photoCal.colorterms.data={} # Name of photometric reference catalog; used to select a color term dict in colorterms. see also applyColorTerms config.fgcmOutputProducts.photoCal.photoCatName=None # Additional magnitude uncertainty to be added in quadrature with measurement errors. config.fgcmOutputProducts.photoCal.magErrFloor=0.003 # Healpix nside to pixelize catalog to compare to reference catalog config.fgcmOutputProducts.referencePixelizationNside=64 # Minimum number of stars per healpix pixel to select for comparisonto the specified reference catalog config.fgcmOutputProducts.referencePixelizationMinStars=200 # Minimum number of stars matched to reference catalog to be used in statistics config.fgcmOutputProducts.referenceMinMatch=50 # Number of healpix pixels to sample to do comparison. Doing too many will take a long time and not yield any more precise results because the final number is the median offset (per band) from the set of pixels. config.fgcmOutputProducts.referencePixelizationNPixels=100 # Version number of the persisted on-disk storage format. # Version 0 had Jy as flux units (default 0 for unversioned catalogs). # Version 1 had nJy as flux units. config.fgcmOutputProducts.datasetConfig.format_version=1 # String to pass to the butler to retrieve persisted files. config.fgcmOutputProducts.datasetConfig.ref_dataset_name='fgcm_stars' # Depth of the HTM tree to make. Default is depth=7 which gives ~ 0.3 sq. deg. per trixel. config.fgcmOutputProducts.datasetConfig.indexer['HTM'].depth=7 config.fgcmOutputProducts.datasetConfig.indexer.name='HTM' # Tolerance on repeatability convergence (per band) config.convergenceTolerance=0.005 # Maximum number of fit cycles config.maxFitCycles=5 # Make plots for debugging purposes? config.doDebuggingPlots=False