LSST Applications 24.1.5,g02d81e74bb+fa3a7a026e,g180d380827+a53a32eff8,g2079a07aa2+86d27d4dc4,g2305ad1205+c0501b3732,g295015adf3+7d3e92f0ec,g2bbee38e9b+0e5473021a,g337abbeb29+0e5473021a,g33d1c0ed96+0e5473021a,g3a166c0a6a+0e5473021a,g3ddfee87b4+5dd1654d75,g48712c4677+3bf1020dcb,g487adcacf7+065c13d9cf,g50ff169b8f+96c6868917,g52b1c1532d+585e252eca,g591dd9f2cf+d7ac436cfb,g5a732f18d5+53520f316c,g64a986408d+fa3a7a026e,g858d7b2824+fa3a7a026e,g8a8a8dda67+585e252eca,g99cad8db69+a5a909b84f,g9ddcbc5298+9a081db1e4,ga1e77700b3+15fc3df1f7,ga8c6da7877+4cf350ccb2,gb0e22166c9+60f28cb32d,gba4ed39666+c2a2e4ac27,gbb8dafda3b+f991a0b59f,gc120e1dc64+9ccbfdb8be,gc28159a63d+0e5473021a,gcf0d15dbbd+5dd1654d75,gd96a1ce819+42fd0ee607,gdaeeff99f8+f9a426f77a,ge6526c86ff+0d71447b4b,ge79ae78c31+0e5473021a,gee10cc3b42+585e252eca,gff1a9f87cc+fa3a7a026e
LSST Data Management Base Package
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Public Member Functions | |
__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 40 of file applyApCorr.py.
lsst.meas.base.applyApCorr.ApCorrInfo.__init__ | ( | self, | |
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name = None ) |
Definition at line 122 of file applyApCorr.py.
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Definition at line 114 of file applyApCorr.py.
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Definition at line 118 of file applyApCorr.py.
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Definition at line 110 of file applyApCorr.py.
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Definition at line 84 of file applyApCorr.py.
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Definition at line 106 of file applyApCorr.py.
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Definition at line 102 of file applyApCorr.py.
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Definition at line 94 of file applyApCorr.py.
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Definition at line 98 of file applyApCorr.py.
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Definition at line 90 of file applyApCorr.py.
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Definition at line 76 of file applyApCorr.py.
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Definition at line 80 of file applyApCorr.py.
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Definition at line 72 of file applyApCorr.py.