LSST Applications 27.0.0,g0265f82a02+469cd937ee,g02d81e74bb+21ad69e7e1,g1470d8bcf6+cbe83ee85a,g2079a07aa2+e67c6346a6,g212a7c68fe+04a9158687,g2305ad1205+94392ce272,g295015adf3+81dd352a9d,g2bbee38e9b+469cd937ee,g337abbeb29+469cd937ee,g3939d97d7f+72a9f7b576,g487adcacf7+71499e7cba,g50ff169b8f+5929b3527e,g52b1c1532d+a6fc98d2e7,g591dd9f2cf+df404f777f,g5a732f18d5+be83d3ecdb,g64a986408d+21ad69e7e1,g858d7b2824+21ad69e7e1,g8a8a8dda67+a6fc98d2e7,g99cad8db69+f62e5b0af5,g9ddcbc5298+d4bad12328,ga1e77700b3+9c366c4306,ga8c6da7877+71e4819109,gb0e22166c9+25ba2f69a1,gb6a65358fc+469cd937ee,gbb8dafda3b+69d3c0e320,gc07e1c2157+a98bf949bb,gc120e1dc64+615ec43309,gc28159a63d+469cd937ee,gcf0d15dbbd+72a9f7b576,gdaeeff99f8+a38ce5ea23,ge6526c86ff+3a7c1ac5f1,ge79ae78c31+469cd937ee,gee10cc3b42+a6fc98d2e7,gf1cff7945b+21ad69e7e1,gfbcc870c63+9a11dc8c8f
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.