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 | |
getExecutionOrder (cls) | |
calculate (self, diaObjects, diaSources, filterDiaSources, band, **kwargs) | |
Static Public Attributes | |
ConfigClass = WeightedMeanDiaPsfFluxConfig | |
list | outputCols = ["scienceFluxMean", "scienceFluxMeanErr"] |
str | plugType = "multi" |
bool | needsFilter = True |
Compute the weighted mean and mean error on the point source fluxes forced photometered at the DiaSource location in the calibrated image. Additionally store number of usable data points.
Definition at line 1007 of file diaCalculationPlugins.py.
lsst.meas.base.diaCalculationPlugins.WeightedMeanDiaTotFlux.calculate | ( | self, | |
diaObjects, | |||
diaSources, | |||
filterDiaSources, | |||
band, | |||
** | kwargs ) |
Compute the weighted mean and mean error of the point source flux. Parameters ---------- diaObject : `dict` Summary object to store values in. diaSources : `pandas.DataFrame` DataFrame representing all diaSources associated with this diaObject. filterDiaSources : `pandas.DataFrame` DataFrame representing diaSources associated with this diaObject that are observed in the band pass ``band``. band : `str` Simple, string name of the filter for the flux being calculated. **kwargs Any additional keyword arguments that may be passed to the plugin.
Reimplemented from lsst.meas.base.diaCalculation.DiaObjectCalculationPlugin.
Definition at line 1025 of file diaCalculationPlugins.py.
lsst.meas.base.diaCalculationPlugins.WeightedMeanDiaTotFlux.getExecutionOrder | ( | cls | ) |
Used to set the relative order of plugin execution. The values returned by `getExecutionOrder` are compared across all plugins, and smaller numbers run first. Notes ----- `CatalogCalculationPlugin`\s must run with `BasePlugin.DEFAULT_CATALOGCALCULATION` or higher. All plugins must implement this method with an appropriate run level
Reimplemented from lsst.meas.base.catalogCalculation.CatalogCalculationPlugin.
Definition at line 1020 of file diaCalculationPlugins.py.
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static |
Definition at line 1014 of file diaCalculationPlugins.py.
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static |
Definition at line 1017 of file diaCalculationPlugins.py.
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static |
Definition at line 1015 of file diaCalculationPlugins.py.
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static |
Definition at line 1016 of file diaCalculationPlugins.py.