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 | |
apply (self, catalog) | |
Static Public Attributes | |
fluxField | |
Select sources using a magnitude limit Note that this assumes that a zero-point has already been applied and the fluxes are in AB fluxes in Jansky. It is therefore principally intended for reference catalogs rather than catalogs extracted from science images. This object can be used as a `lsst.pex.config.Config` for configuring the limit, and then the `apply` method can be used to identify sources in the catalog that match the configured limit.
Definition at line 273 of file sourceSelector.py.
lsst.meas.algorithms.sourceSelector.MagnitudeLimit.apply | ( | self, | |
catalog ) |
Apply the magnitude limits to a catalog Parameters ---------- catalog : `lsst.afw.table.SourceCatalog` Catalog of sources to which the limit will be applied. Returns ------- selected : `numpy.ndarray` Boolean array indicating for each source whether it is selected (True means selected).
Reimplemented from lsst.meas.algorithms.sourceSelector.BaseLimit.
Definition at line 288 of file sourceSelector.py.
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static |
Definition at line 285 of file sourceSelector.py.