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 | readIsrData (self, dataRef, rawExposure) |
def | check (self, exposure) |
def | run (self, exposure, strayLightData) |
def | checkFilter (self, exposure) |
Static Public Attributes | |
ConfigClass = StrayLightConfig | |
Remove stray light from instruments. This is a dummy task to be retargeted with an camera-specific version.
Definition at line 45 of file straylight.py.
def lsst.ip.isr.straylight.StrayLightTask.check | ( | self, | |
exposure | |||
) |
Check if stray light correction should be run. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to correct.
Definition at line 82 of file straylight.py.
def lsst.ip.isr.straylight.StrayLightTask.checkFilter | ( | self, | |
exposure | |||
) |
Check whether we should fringe-subtract the science exposure. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to check the filter of. Returns ------- needsFringe : `bool` If True, then the exposure has a filter listed in the configuration, and should have the fringe applied.
Definition at line 105 of file straylight.py.
def lsst.ip.isr.straylight.StrayLightTask.readIsrData | ( | self, | |
dataRef, | |||
rawExposure | |||
) |
Read and return calibration products relevant for correcting stray light in the given exposure. Parameters ---------- dataRef : `daf.persistence.butlerSubset.ButlerDataRef` Butler reference of the detector data to be processed rawExposure : `afw.image.Exposure` The raw exposure that will later be corrected with the retrieved calibration data; should not be modified in this method. Returns ------- straylightData : `object`, optional An opaque object that should be passed as the second argument to the `run` method. If `None`, no stray light correction will be performed for the given image. Any other object (e.g. `True`) may be used to signal that stray light correction should be performed even if there is nothing to read. Notes ----- This method will be called only when `IsrTask` is run by the Gen2 Middleware (i.e. CmdLineTask).
Definition at line 53 of file straylight.py.
def lsst.ip.isr.straylight.StrayLightTask.run | ( | self, | |
exposure, | |||
strayLightData | |||
) |
Correct stray light. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to correct. strayLightData : `object`, optional An opaque object that contains any calibration data used to correct for stray light.
Definition at line 92 of file straylight.py.
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static |
Definition at line 50 of file straylight.py.