|
lsst.ip.isr
14.0-12-g947dc0d+1
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Classes | |
| class | CrosstalkConfig |
| class | CrosstalkTask |
Functions | |
| def | extractAmp (image, amp, corner) |
| def | calculateBackground (mi, badPixels=["BAD"]) |
| def | subtractCrosstalk (exposure, badPixels=["BAD"], minPixelToMask=45000, crosstalkStr="CROSSTALK") |
Variables | |
| dictionary | X_FLIP |
| dictionary | Y_FLIP |
| def lsst.ip.isr.crosstalk.calculateBackground | ( | mi, | |
badPixels = ["BAD"] |
|||
| ) |
Calculate median background in image
Getting a great background model isn't important for crosstalk correction,
since the crosstalk is at a low level. The median should be sufficient.
Parameters
----------
mi : `lsst.afw.image.MaskedImage`
MaskedImage for which to measure background.
badPixels : `list` of `str`
Mask planes to ignore.
Returns
-------
bg : `float`
Median background level.
Definition at line 115 of file crosstalk.py.
| def lsst.ip.isr.crosstalk.extractAmp | ( | image, | |
| amp, | |||
| corner | |||
| ) |
Return an image of the amp
The returned image will have the amp's readout corner in the
nominated `corner`.
Parameters
----------
image : `lsst.afw.image.Image` or `lsst.afw.image.MaskedImage`
Image containing the amplifier of interest.
amp : `lsst.afw.table.AmpInfoRecord`
Amplifier information.
corner : `lsst.afw.table.ReadoutCorner` or `None`
Corner in which to put the amp's readout corner, or `None` for
no flipping.
Returns
-------
output : `lsst.afw.image.Image`
Image of the amplifier in the standard configuration.
Definition at line 86 of file crosstalk.py.
| def lsst.ip.isr.crosstalk.subtractCrosstalk | ( | exposure, | |
badPixels = ["BAD"], |
|||
minPixelToMask = 45000, |
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crosstalkStr = "CROSSTALK" |
|||
| ) |
Subtract the intra-CCD crosstalk from an exposure
We set the mask plane indicated by ``crosstalkStr`` in a target amplifier
for pixels in a source amplifier that exceed `minPixelToMask`. Note that
the correction is applied to all pixels in the amplifier, but only those
that have a substantial crosstalk are masked with ``crosstalkStr``.
The uncorrected image is used as a template for correction. This is good
enough if the crosstalk is small (e.g., coefficients < ~ 1e-3), but if it's
larger you may want to iterate.
Parameters
----------
exposure : `lsst.afw.image.Exposure`
Exposure for which to subtract crosstalk.
badPixels : `list` of `str`
Mask planes to ignore.
minPixelToMask : `float`
Minimum pixel value in source amplifier for which to set
``crosstalkStr`` mask plane in target amplifier.
crosstalkStr : `str`
Mask plane name for pixels greatly modified by crosstalk.
Definition at line 139 of file crosstalk.py.
| dictionary lsst.ip.isr.crosstalk.X_FLIP |
Definition at line 80 of file crosstalk.py.
| dictionary lsst.ip.isr.crosstalk.Y_FLIP |
Definition at line 82 of file crosstalk.py.
1.8.13