LSST Applications
21.0.0+04719a4bac,21.0.0-1-ga51b5d4+f5e6047307,21.0.0-11-g2b59f77+a9c1acf22d,21.0.0-11-ga42c5b2+86977b0b17,21.0.0-12-gf4ce030+76814010d2,21.0.0-13-g1721dae+760e7a6536,21.0.0-13-g3a573fe+768d78a30a,21.0.0-15-g5a7caf0+f21cbc5713,21.0.0-16-g0fb55c1+b60e2d390c,21.0.0-19-g4cded4ca+71a93a33c0,21.0.0-2-g103fe59+bb20972958,21.0.0-2-g45278ab+04719a4bac,21.0.0-2-g5242d73+3ad5d60fb1,21.0.0-2-g7f82c8f+8babb168e8,21.0.0-2-g8f08a60+06509c8b61,21.0.0-2-g8faa9b5+616205b9df,21.0.0-2-ga326454+8babb168e8,21.0.0-2-gde069b7+5e4aea9c2f,21.0.0-2-gecfae73+1d3a86e577,21.0.0-2-gfc62afb+3ad5d60fb1,21.0.0-25-g1d57be3cd+e73869a214,21.0.0-3-g357aad2+ed88757d29,21.0.0-3-g4a4ce7f+3ad5d60fb1,21.0.0-3-g4be5c26+3ad5d60fb1,21.0.0-3-g65f322c+e0b24896a3,21.0.0-3-g7d9da8d+616205b9df,21.0.0-3-ge02ed75+a9c1acf22d,21.0.0-4-g591bb35+a9c1acf22d,21.0.0-4-g65b4814+b60e2d390c,21.0.0-4-gccdca77+0de219a2bc,21.0.0-4-ge8a399c+6c55c39e83,21.0.0-5-gd00fb1e+05fce91b99,21.0.0-6-gc675373+3ad5d60fb1,21.0.0-64-g1122c245+4fb2b8f86e,21.0.0-7-g04766d7+cd19d05db2,21.0.0-7-gdf92d54+04719a4bac,21.0.0-8-g5674e7b+d1bd76f71f,master-gac4afde19b+a9c1acf22d,w.2021.13
LSST Data Management Base Package
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Public Member Functions | |
def | __init__ (self, schema, model, name=None) |
Static Public Attributes | |
name = None | |
modelName = None | |
modelSigmaName = None | |
doApCorrColumn = None | |
instFluxName = None | |
instFluxErrName = None | |
instFluxKey = None | |
instFluxErrKey = None | |
fluxFlagKey = None | |
apCorrKey = None | |
apCorrErrKey = None | |
apCorrFlagKey = None | |
Catalog field names and keys needed to aperture correct a particular instrument flux. Parameters ---------- schema : `lsst.afw.table` Source catalog schema. Three fields are used to generate keys: - ``{name}_instFlux`` - ``{name}_instFluxErr`` - ``{name}_flag`` Three fields are added: - ``{name}_apCorr`` (only if not already added by proxy) - ``{name}_apCorrErr`` (only if not already added by proxy) - ``{name}_flag_apCorr`` model : `str` Field name prefix for instFlux with aperture correction model, e.g. "base_PsfFlux" name : `str` Field name prefix for instFlux needing aperture correction; may be `None` if it is the same as ``model`` Notes ----- The aperture correction can be derived from the meaasurements in the column being aperture-corrected or from measurements in a different column (a "proxy"). In the first case, we will add columns to contain the aperture correction values; in the second case (using a proxy), we will add an alias to the proxy's aperture correction values. In all cases, we add a flag.
Definition at line 41 of file applyApCorr.py.
def lsst.meas.base.applyApCorr.ApCorrInfo.__init__ | ( | self, | |
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name = None |
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Definition at line 123 of file applyApCorr.py.
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Definition at line 115 of file applyApCorr.py.
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Definition at line 119 of file applyApCorr.py.
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Definition at line 111 of file applyApCorr.py.
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Definition at line 85 of file applyApCorr.py.
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Definition at line 107 of file applyApCorr.py.
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Definition at line 103 of file applyApCorr.py.
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Definition at line 95 of file applyApCorr.py.
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Definition at line 99 of file applyApCorr.py.
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Definition at line 91 of file applyApCorr.py.
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Definition at line 77 of file applyApCorr.py.
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Definition at line 81 of file applyApCorr.py.
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Definition at line 73 of file applyApCorr.py.