LSST Applications
21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
LSST Data Management Base Package
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Public Member Functions | |
def | factory (cls, stamp_im, metadata, idx, archive_element=None) |
def | measureAndNormalize (self, annulus, statsControl=afwMath.StatisticsControl(), statsFlag=afwMath.stringToStatisticsProperty("MEAN"), badMaskPlanes=('BAD', 'SAT', 'NO_DATA')) |
Public Attributes | |
annularFlux | |
Single stamp centered on a bright star, normalized by its annularFlux. Parameters ---------- stamp_im : `lsst.afw.image.MaskedImage` Pixel data for this postage stamp position : `lsst.geom.Point2I` Origin of the stamps in its origin exposure (pixels) gaiaGMag : `float` Gaia G magnitude for the object in this stamp gaiaId : `int` Gaia object identifier annularFlux : `Optional[float]` Flux in an annulus around the object
Definition at line 42 of file brightStarStamps.py.
def lsst.meas.algorithms.brightStarStamps.BrightStarStamp.factory | ( | cls, | |
stamp_im, | |||
metadata, | |||
idx, | |||
archive_element = None |
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) |
This method is needed to service the FITS reader. We need a standard interface to construct objects like this. Parameters needed to construct this object are passed in via a metadata dictionary and then passed to the constructor of this class. This particular factory method requires keys: G_MAGS, GAIA_IDS, and ANNULAR_FLUXES. They should each point to lists of values. Parameters ---------- stamp_im : `lsst.afw.image.MaskedImage` Pixel data to pass to the constructor metadata : `dict` Dictionary containing the information needed by the constructor. idx : `int` Index into the lists in ``metadata`` archive_element : `lsst.afwTable.io.Persistable`, optional Archive element (e.g. Transform or WCS) associated with this stamp. Returns ------- brightstarstamp : `BrightStarStamp` An instance of this class
Reimplemented from lsst.meas.algorithms.stamps.AbstractStamp.
Definition at line 67 of file brightStarStamps.py.
def lsst.meas.algorithms.brightStarStamps.BrightStarStamp.measureAndNormalize | ( | self, | |
annulus, | |||
statsControl = afwMath.StatisticsControl() , |
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statsFlag = afwMath.stringToStatisticsProperty("MEAN") , |
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badMaskPlanes = ('BAD', 'SAT', 'NO_DATA') |
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) |
Compute "annularFlux", the integrated flux within an annulus around an object's center, and normalize it. Since the center of bright stars are saturated and/or heavily affected by ghosts, we measure their flux in an annulus with a large enough inner radius to avoid the most severe ghosts and contain enough non-saturated pixels. Parameters ---------- annulus : `lsst.afw.geom.spanSet.SpanSet` SpanSet containing the annulus to use for normalization. statsControl : `lsst.afw.math.statistics.StatisticsControl`, optional StatisticsControl to be used when computing flux over all pixels within the annulus. statsFlag : `lsst.afw.math.statistics.Property`, optional statsFlag to be passed on to ``afwMath.makeStatistics`` to compute annularFlux. Defaults to a simple MEAN. badMaskPlanes : `collections.abc.Collection` [`str`] Collection of mask planes to ignore when computing annularFlux.
Definition at line 106 of file brightStarStamps.py.
lsst.meas.algorithms.brightStarStamps.BrightStarStamp.annularFlux |
Definition at line 143 of file brightStarStamps.py.