LSST Applications 24.1.6,g063fba187b+56b85ce14a,g0f08755f38+df8a265115,g12f32b3c4e+891a09f10d,g1524ad2192+7a5d7b3fbd,g1653933729+a8ce1bb630,g168dd56ebc+a8ce1bb630,g28da252d5a+07cb1400be,g2bbee38e9b+ae03bbfc84,g2bc492864f+ae03bbfc84,g3156d2b45e+6e55a43351,g347aa1857d+ae03bbfc84,g35bb328faa+a8ce1bb630,g3a166c0a6a+ae03bbfc84,g3e281a1b8c+c5dd892a6c,g414038480c+6b9177ef31,g41af890bb2+8f257c4c0b,g781aacb6e4+a8ce1bb630,g7af13505b9+7137b3b17d,g80478fca09+6df6903293,g82479be7b0+091ce1d07f,g858d7b2824+df8a265115,g89c8672015+f4add4ffd5,g9125e01d80+a8ce1bb630,g9726552aa6+414189b318,ga5288a1d22+4a2bca08d7,gacef1a1666+c9a8ff65f4,gb58c049af0+d64f4d3760,gbcfae0f0a0+de1d42d831,gc28159a63d+ae03bbfc84,gcf0d15dbbd+72117bf34e,gda6a2b7d83+72117bf34e,gdaeeff99f8+1711a396fd,ge500cccec5+c8c9c9af63,ge79ae78c31+ae03bbfc84,gf0baf85859+c1f95f4921,gfa517265be+df8a265115,gfa999e8aa5+17cd334064,gfb92a5be7c+df8a265115
LSST Data Management Base Package
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Public Member Functions | Static Public Attributes | List of all members
lsst.meas.algorithms.sourceSelector.MagnitudeLimit Class Reference
Inheritance diagram for lsst.meas.algorithms.sourceSelector.MagnitudeLimit:
lsst.meas.algorithms.sourceSelector.BaseLimit

Public Member Functions

 apply (self, catalog)
 

Static Public Attributes

 fluxField
 

Detailed Description

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 274 of file sourceSelector.py.

Member Function Documentation

◆ apply()

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 289 of file sourceSelector.py.

289 def apply(self, catalog):
290 """Apply the magnitude limits to a catalog
291
292 Parameters
293 ----------
294 catalog : `lsst.afw.table.SourceCatalog`
295 Catalog of sources to which the limit will be applied.
296
297 Returns
298 -------
299 selected : `numpy.ndarray`
300 Boolean array indicating for each source whether it is selected
301 (True means selected).
302 """
303 flagField = self.fluxField + "_flag"
304 selected = np.logical_not(_getFieldFromCatalog(catalog, flagField, isFlag=True))
305 flux = _getFieldFromCatalog(catalog, self.fluxField)
306
307 magnitude = (flux*u.nJy).to_value(u.ABmag)
308 selected &= BaseLimit.apply(self, magnitude)
309 return selected
310
311

Member Data Documentation

◆ fluxField

lsst.meas.algorithms.sourceSelector.MagnitudeLimit.fluxField
static
Initial value:
= pexConfig.Field(dtype=str, default="flux",
doc="Name of the source flux field to use.")

Definition at line 286 of file sourceSelector.py.


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