LSST Applications
21.0.0-147-g0e635eb1+1acddb5be5,22.0.0+052faf71bd,22.0.0+1ea9a8b2b2,22.0.0+6312710a6c,22.0.0+729191ecac,22.0.0+7589c3a021,22.0.0+9f079a9461,22.0.1-1-g7d6de66+b8044ec9de,22.0.1-1-g87000a6+536b1ee016,22.0.1-1-g8e32f31+6312710a6c,22.0.1-10-gd060f87+016f7cdc03,22.0.1-12-g9c3108e+df145f6f68,22.0.1-16-g314fa6d+c825727ab8,22.0.1-19-g93a5c75+d23f2fb6d8,22.0.1-19-gb93eaa13+aab3ef7709,22.0.1-2-g8ef0a89+b8044ec9de,22.0.1-2-g92698f7+9f079a9461,22.0.1-2-ga9b0f51+052faf71bd,22.0.1-2-gac51dbf+052faf71bd,22.0.1-2-gb66926d+6312710a6c,22.0.1-2-gcb770ba+09e3807989,22.0.1-20-g32debb5+b8044ec9de,22.0.1-23-gc2439a9a+fb0756638e,22.0.1-3-g496fd5d+09117f784f,22.0.1-3-g59f966b+1e6ba2c031,22.0.1-3-g849a1b8+f8b568069f,22.0.1-3-gaaec9c0+c5c846a8b1,22.0.1-32-g5ddfab5d3+60ce4897b0,22.0.1-4-g037fbe1+64e601228d,22.0.1-4-g8623105+b8044ec9de,22.0.1-5-g096abc9+d18c45d440,22.0.1-5-g15c806e+57f5c03693,22.0.1-7-gba73697+57f5c03693,master-g6e05de7fdc+c1283a92b8,master-g72cdda8301+729191ecac,w.2021.39
LSST Data Management Base Package
|
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, | |
schema, | |||
model, | |||
name = None |
|||
) |
Definition at line 123 of file applyApCorr.py.
|
static |
Definition at line 115 of file applyApCorr.py.
|
static |
Definition at line 119 of file applyApCorr.py.
|
static |
Definition at line 111 of file applyApCorr.py.
|
static |
Definition at line 85 of file applyApCorr.py.
|
static |
Definition at line 107 of file applyApCorr.py.
|
static |
Definition at line 103 of file applyApCorr.py.
|
static |
Definition at line 95 of file applyApCorr.py.
|
static |
Definition at line 99 of file applyApCorr.py.
|
static |
Definition at line 91 of file applyApCorr.py.
|
static |
Definition at line 77 of file applyApCorr.py.
|
static |
Definition at line 81 of file applyApCorr.py.
|
static |
Definition at line 73 of file applyApCorr.py.