LSST Applications
21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
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.