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 | Static Public Attributes | List of all members
lsst.meas.algorithms.sourceSelector.ColorLimit Class Reference
Inheritance diagram for lsst.meas.algorithms.sourceSelector.ColorLimit:
lsst.meas.algorithms.sourceSelector.BaseLimit

Public Member Functions

 apply (self, catalog)
 

Static Public Attributes

 primary = pexConfig.Field(dtype=str, doc="Name of column with primary flux measurement")
 
 secondary = pexConfig.Field(dtype=str, doc="Name of column with secondary flux measurement")
 

Detailed Description

Select sources using a color limit

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.

We refer to 'primary' and 'secondary' flux measurements; these are the
two components of the color, which is:

    instFluxToMag(cat[primary]) - instFluxToMag(cat[secondary])

Definition at line 201 of file sourceSelector.py.

Member Function Documentation

◆ apply()

lsst.meas.algorithms.sourceSelector.ColorLimit.apply ( self,
catalog )
Apply the color limit to a catalog

Parameters
----------
catalog : Various table formats
    Catalog of sources to which the limit will be applied.
    Supports `lsst.afw.table.SourceCatalog` or `pandas.DataFrame`
    or `astropy.table.Table`

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 216 of file sourceSelector.py.

216 def apply(self, catalog):
217 """Apply the color limit to a catalog
218
219 Parameters
220 ----------
221 catalog : Various table formats
222 Catalog of sources to which the limit will be applied.
223 Supports `lsst.afw.table.SourceCatalog` or `pandas.DataFrame`
224 or `astropy.table.Table`
225
226 Returns
227 -------
228 selected : `numpy.ndarray`
229 Boolean array indicating for each source whether it is selected
230 (True means selected).
231 """
232 primary = _getFieldFromCatalog(catalog, self.primary)
233 secondary = _getFieldFromCatalog(catalog, self.secondary)
234
235 primary = (primary*u.nJy).to_value(u.ABmag)
236 secondary = (secondary*u.nJy).to_value(u.ABmag)
237 color = primary - secondary
238 return BaseLimit.apply(self, color)
239
240

Member Data Documentation

◆ primary

lsst.meas.algorithms.sourceSelector.ColorLimit.primary = pexConfig.Field(dtype=str, doc="Name of column with primary flux measurement")
static

Definition at line 213 of file sourceSelector.py.

◆ secondary

lsst.meas.algorithms.sourceSelector.ColorLimit.secondary = pexConfig.Field(dtype=str, doc="Name of column with secondary flux measurement")
static

Definition at line 214 of file sourceSelector.py.


The documentation for this class was generated from the following file: