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lsst.ip.isr gd2a69bfd97+d18973ec71
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Public Member Functions | |
| __init__ (self, **kwargs) | |
| run (self) | |
| makeData (self) | |
| makeBfKernel (self) | |
| makeElectrostaticBf (self) | |
| makeDeferredChargeCalib (self) | |
| makeDefectList (self) | |
| makeCrosstalkCoeff (self) | |
| makeTransmissionCurve (self) | |
| makeLinearity (self) | |
| makeImage (self) | |
| getCamera (self, isForAssembly=False) | |
| getExposure (self, isTrimmed=None) | |
| getWcs (self) | |
| localCoordToExpCoord (self, ampData, x, y) | |
| amplifierAddNoise (self, ampData, mean, sigma, rng=None) | |
| amplifierAddYGradient (self, ampData, start, end) | |
| amplifierAddSource (self, ampData, scale, x0, y0) | |
| amplifierAddFringe (self, amp, ampData, scale, x0=100, y0=0) | |
| amplifierMultiplyFlat (self, amp, ampData, fracDrop, u0=100.0, v0=100.0) | |
Public Attributes | |
| rng = np.random.RandomState(self.config.rngSeed) | |
| crosstalkCoeffs | |
| float | bfKernel |
| int | aN |
| int | aE |
| int | aS = self.aN |
| int | aW = self.aE |
| tuple | aVector = (self.aN, self.aS, self.aE, self.aW) |
Static Public Attributes | |
| ConfigClass = IsrMockConfig | |
Protected Attributes | |
| _display | |
Static Protected Attributes | |
| str | _DefaultName = "isrMock" |
Generate a raw exposure dict suitable for ISR.
Definition at line 989 of file isrMock.py.
| lsst.ip.isr.isrMock.RawDictMock.__init__ | ( | self, | |
| ** | kwargs ) |
Definition at line 992 of file isrMock.py.
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inherited |
Add a fringe-like ripple pattern to an amplifier's image data.
Parameters
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amp : `~lsst.afw.ampInfo.AmpInfoRecord`
Amplifier to operate on. Needed for amp<->exp coordinate
transforms.
ampData : `lsst.afw.image.ImageF`
Amplifier image to operate on.
scale : `numpy.array` or `float`
Peak intensity scaling for the ripple.
x0 : `numpy.array` or `float`, optional
Fringe center
y0 : `numpy.array` or `float`, optional
Fringe center
Notes
-----
This uses an offset sinc function to generate a ripple
pattern. True fringes have much finer structure, but this
pattern should be visually identifiable. The (x, y)
coordinates are in the frame of the amplifier, and (u, v) in
the frame of the full trimmed image.
Definition at line 875 of file isrMock.py.
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inherited |
Add Gaussian noise to an amplifier's image data.
This method operates in the amplifier coordinate frame.
Parameters
----------
ampData : `lsst.afw.image.ImageF`
Amplifier image to operate on.
mean : `float`
Mean value of the Gaussian noise.
sigma : `float`
Sigma of the Gaussian noise.
rng : `np.random.RandomState`, optional
Random state to use instead of self.rng.
Definition at line 809 of file isrMock.py.
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inherited |
Add a single Gaussian source to an amplifier.
This method operates in the amplifier coordinate frame.
Parameters
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ampData : `lsst.afw.image.ImageF`
Amplifier image to operate on.
scale : `float`
Peak flux of the source to add.
x0 : `float`
X-coordinate of the source peak.
y0 : `float`
Y-coordinate of the source peak.
Definition at line 853 of file isrMock.py.
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inherited |
Add a y-axis linear gradient to an amplifier's image data.
This method operates in the amplifier coordinate frame.
Parameters
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ampData : `lsst.afw.image.ImageF`
Amplifier image to operate on.
start : `float`
Start value of the gradient (at y=0).
end : `float`
End value of the gradient (at y=ymax).
Definition at line 834 of file isrMock.py.
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inherited |
Multiply an amplifier's image data by a flat-like pattern.
Parameters
----------
amp : `lsst.afw.ampInfo.AmpInfoRecord`
Amplifier to operate on. Needed for amp<->exp coordinate
transforms.
ampData : `lsst.afw.image.ImageF`
Amplifier image to operate on.
fracDrop : `float`
Fractional drop from center to edge of detector along x-axis.
u0 : `float`
Peak location in detector coordinates.
v0 : `float`
Peak location in detector coordinates.
Notes
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This uses a 2-d Gaussian to simulate an illumination pattern
that falls off towards the edge of the detector. The (x, y)
coordinates are in the frame of the amplifier, and (u, v) in
the frame of the full trimmed image.
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 907 of file isrMock.py.
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inherited |
Construct a test camera object.
Parameters
-------
isForAssembly : `bool`
If True, construct a camera with "super raw"
orientation (all amplifiers have LL readout
corner but still contains the necessary flip
and offset info needed for assembly. This is
needed if isLsstLike is True. If False, return
a camera with bboxes flipped and offset to the
correct orientation given the readout corner.
Returns
-------
camera : `lsst.afw.cameraGeom.camera`
Test camera.
Definition at line 596 of file isrMock.py.
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inherited |
Construct a test exposure.
The test exposure has a simple WCS set, as well as a list of
unlikely header keywords that can be removed during ISR
processing to exercise that code.
Parameters
----------
isTrimmed : `bool` or `None`, optional
Override the configuration isTrimmed?
Returns
-------
exposure : `lsst.afw.exposure.Exposure`
Construct exposure containing masked image of the
appropriate size.
Definition at line 623 of file isrMock.py.
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inherited |
Construct a dummy WCS object.
Taken from the deprecated ip_isr/examples/exampleUtils.py.
This is not guaranteed, given the distortion and pixel scale
listed in the afwTestUtils camera definition.
Returns
-------
wcs : `lsst.afw.geom.SkyWcs`
Test WCS transform.
Definition at line 761 of file isrMock.py.
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inherited |
Convert between a local amplifier coordinate and the full
exposure coordinate.
Parameters
----------
ampData : `lsst.afw.image.ImageF`
Amplifier image to use for conversions.
x : `int`
X-coordinate of the point to transform.
y : `int`
Y-coordinate of the point to transform.
Returns
-------
u : `int`
Transformed x-coordinate.
v : `int`
Transformed y-coordinate.
Notes
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The output is transposed intentionally here, to match the
internal transpose between numpy and afw.image coordinates.
Definition at line 778 of file isrMock.py.
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inherited |
Generate a simple Gaussian brighter-fatter kernel.
Returns
-------
kernel : `numpy.ndarray`
Simulated brighter-fatter kernel.
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 401 of file isrMock.py.
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inherited |
Generate the simulated crosstalk coefficients.
Returns
-------
coeffs : `numpy.ndarray`
Simulated crosstalk coefficients.
Definition at line 438 of file isrMock.py.
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inherited |
Generate simulated ISR data.
Currently, only the class defined crosstalk coefficient
matrix, brighter-fatter kernel, a constant unity transmission
curve, or a simple single-entry defect list can be generated.
Returns
-------
dataProduct :
Simulated ISR data product.
Definition at line 361 of file isrMock.py.
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inherited |
Generate a simple single-entry defect list.
Returns
-------
defectList : `lsst.meas.algorithms.Defects`
Simulated defect list
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 427 of file isrMock.py.
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inherited |
Generate a CTI calibration.
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 421 of file isrMock.py.
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inherited |
Generate a simple Gaussian brighter-fatter kernel.
Returns
-------
kernel : `numpy.ndarray`
Simulated brighter-fatter kernel.
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 411 of file isrMock.py.
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inherited |
Generate a simulated ISR image.
Returns
-------
exposure : `lsst.afw.image.Exposure` or `dict`
Simulated ISR image data.
Notes
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This method currently constructs a "raw" data image by:
* Generating a simulated sky with noise
* Adding a single Gaussian "star"
* Adding the fringe signal
* Multiplying the frame by the simulated flat
* Adding dark current (and noise)
* Adding a bias offset (and noise)
* Adding an overscan gradient parallel to the pixel y-axis
* Simulating crosstalk by adding a scaled version of each
amplifier to each other amplifier.
The exposure with image data constructed this way is in one of
three formats.
* A single image, with overscan and prescan regions retained
* A single image, with overscan and prescan regions trimmed
* A `dict`, containing the amplifer data indexed by the
amplifier name.
The nonlinearity, CTE, and brighter fatter are currently not
implemented.
Note that this method generates an image in the reverse
direction as the ISR processing, as the output image here has
had a series of instrument effects added to an idealized
exposure.
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 469 of file isrMock.py.
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inherited |
Generate a linearity dataset. Returns ------- linearizer : `lsst.ip.isr.Linearizer`
Definition at line 460 of file isrMock.py.
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inherited |
Generate a simulated flat transmission curve.
Returns
-------
transmission : `lsst.afw.image.TransmissionCurve`
Simulated transmission curve.
Definition at line 449 of file isrMock.py.
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inherited |
Generate a mock ISR product, and return it.
Returns
-------
image : `lsst.afw.image.Exposure`
Simulated ISR image with signals added.
dataProduct :
Simulated ISR data products.
None :
Returned if no valid configuration was found.
Raises
------
RuntimeError
Raised if both doGenerateImage and doGenerateData are specified.
Reimplemented in lsst.ip.isr.isrMockLSST.IsrMockLSST.
Definition at line 335 of file isrMock.py.
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Definition at line 292 of file isrMock.py.
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Definition at line 307 of file isrMock.py.
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Definition at line 327 of file isrMock.py.
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Definition at line 323 of file isrMock.py.
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Definition at line 331 of file isrMock.py.
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Definition at line 333 of file isrMock.py.
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Definition at line 332 of file isrMock.py.
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Definition at line 317 of file isrMock.py.
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Definition at line 291 of file isrMock.py.
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Definition at line 299 of file isrMock.py.
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Definition at line 296 of file isrMock.py.