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lsst.ip.isr gbffcd5fa91+39a08c657f
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Public Member Functions | |
| loadFringes (self, fringeExp, expId=None, assembler=None) | |
| run (self, exposure, fringes, seed=None) | |
| checkFilter (self, exposure) | |
| removePedestal (self, fringe) | |
| generatePositions (self, exposure, rng) | |
| measureExposure (self, exposure, positions, title="Fringe") | |
| solve (self, science, fringes) | |
| subtract (self, science, fringes, solution) | |
Static Public Attributes | |
| ConfigClass = FringeConfig | |
Protected Member Functions | |
| _solve (self, science, fringes) | |
Static Protected Attributes | |
| str | _DefaultName = 'isrFringe' |
Task to remove fringes from a science exposure We measure fringe amplitudes at random positions on the science exposure and at the same positions on the (potentially multiple) fringe frames and solve for the scales simultaneously.
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protected |
Solve for the scale factors.
Parameters
----------
science : `numpy.array`
Array of measured science image values at each of the
positions supplied.
fringes : `numpy.array`
Array of measured fringe values at each of the positions
supplied.
Returns
-------
solution : `np.array`
Fringe solution amplitudes for each input fringe frame.
| lsst.ip.isr.fringe.FringeTask.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.
| lsst.ip.isr.fringe.FringeTask.generatePositions | ( | self, | |
| exposure, | |||
| rng ) |
Generate a random distribution of positions for measuring fringe
amplitudes.
Parameters
----------
exposure : `lsst.afw.image.Exposure`
Exposure to measure the positions on.
rng : `numpy.random.RandomState`
Random number generator to use.
Returns
-------
positions : `numpy.array`
Two-dimensional array containing the positions to sample
for fringe amplitudes.
| lsst.ip.isr.fringe.FringeTask.loadFringes | ( | self, | |
| fringeExp, | |||
| expId = None, | |||
| assembler = None ) |
Pack the fringe data into a Struct.
This method moves the struct parsing code into a butler
generation agnostic handler.
Parameters
----------
fringeExp : `lsst.afw.exposure.Exposure`
The exposure containing the fringe data.
expId : `int`, optional
Exposure id to be fringe corrected, used to set RNG seed.
assembler : `lsst.ip.isr.AssembleCcdTask`, optional
An instance of AssembleCcdTask (for assembling fringe
frames).
Returns
-------
fringeData : `pipeBase.Struct`
Struct containing fringe data:
``fringes``
Calibration fringe files containing master fringe frames.
( : `lsst.afw.image.Exposure` or `list` thereof)
``seed``
Seed for random number generation. (`int`, optional)
| lsst.ip.isr.fringe.FringeTask.measureExposure | ( | self, | |
| exposure, | |||
| positions, | |||
| title = "Fringe" ) |
Measure fringe amplitudes for an exposure
The fringe amplitudes are measured as the statistic within a square
aperture. The statistic within a larger aperture are subtracted so
as to remove the background.
Parameters
----------
exposure : `lsst.afw.image.Exposure`
Exposure to measure the positions on.
positions : `numpy.array`
Two-dimensional array containing the positions to sample
for fringe amplitudes.
title : `str`, optional
Title used for debug out plots.
Returns
-------
fringes : `numpy.array`
Array of measured exposure values at each of the positions
supplied.
| lsst.ip.isr.fringe.FringeTask.removePedestal | ( | self, | |
| fringe ) |
| lsst.ip.isr.fringe.FringeTask.run | ( | self, | |
| exposure, | |||
| fringes, | |||
| seed = None ) |
Remove fringes from the provided science exposure.
Primary method of FringeTask. Fringes are only subtracted if the
science exposure has a filter listed in the configuration.
Parameters
----------
exposure : `lsst.afw.image.Exposure`
Science exposure from which to remove fringes.
fringes : `lsst.afw.image.Exposure` or `list` thereof
Calibration fringe files containing master fringe frames.
seed : `int`, optional
Seed for random number generation.
Returns
-------
solution : `np.array`
Fringe solution amplitudes for each input fringe frame.
rms : `float`
RMS error for the fit solution for this exposure.
| lsst.ip.isr.fringe.FringeTask.solve | ( | self, | |
| science, | |||
| fringes ) |
Solve for the scale factors with iterative clipping.
Parameters
----------
science : `numpy.array`
Array of measured science image values at each of the
positions supplied.
fringes : `numpy.array`
Array of measured fringe values at each of the positions
supplied.
Returns
-------
solution : `np.array`
Fringe solution amplitudes for each input fringe frame.
rms : `float`
RMS error for the fit solution for this exposure.
| lsst.ip.isr.fringe.FringeTask.subtract | ( | self, | |
| science, | |||
| fringes, | |||
| solution ) |
Subtract the fringes.
Parameters
----------
science : `lsst.afw.image.Exposure`
Science exposure from which to remove fringes.
fringes : `lsst.afw.image.Exposure` or `list` thereof
Calibration fringe files containing master fringe frames.
solution : `np.array`
Fringe solution amplitudes for each input fringe frame.
Raises
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RuntimeError
Raised if the number of fringe frames does not match the
number of measured amplitudes.
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staticprotected |
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