LSST Applications g0fba68d861+bb7a7cfa1f,g1ec0fe41b4+f536777771,g1fd858c14a+470a99fdf4,g216c3ac8a7+0d4d80193f,g35bb328faa+fcb1d3bbc8,g4d2262a081+23bd310d1b,g53246c7159+fcb1d3bbc8,g56a49b3a55+369644a549,g5a012ec0e7+3632fc3ff3,g60b5630c4e+3bfb9058a5,g67b6fd64d1+ed4b5058f4,g78460c75b0+2f9a1b4bcd,g786e29fd12+cf7ec2a62a,g8180f54f50+60bd39f3b6,g8352419a5c+fcb1d3bbc8,g87d29937c9+57a68d035f,g8852436030+4699110379,g89139ef638+ed4b5058f4,g9125e01d80+fcb1d3bbc8,g94187f82dc+3bfb9058a5,g989de1cb63+ed4b5058f4,g9ccd5d7f00+b7cae620c0,g9d31334357+3bfb9058a5,g9f33ca652e+00883ace41,gabe3b4be73+1e0a283bba,gabf8522325+fa80ff7197,gb1101e3267+27b24065a3,gb58c049af0+f03b321e39,gb89ab40317+ed4b5058f4,gc0af124501+708fe67c54,gcf25f946ba+4699110379,gd6cbbdb0b4+bb83cc51f8,gde0f65d7ad+acd5afb0eb,ge1ad929117+3bfb9058a5,ge278dab8ac+d65b3c2b70,ge410e46f29+ed4b5058f4,gf5e32f922b+fcb1d3bbc8,gf67bdafdda+ed4b5058f4,w.2025.17
LSST Data Management Base Package
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Public Member Functions | |
__init__ (self, detector=None, nAmp=0, **kwargs) | |
updateMetadata (self, setDate=False, **kwargs) | |
fromDetector (self, detector, coeffVector=None, coeffSqrVector=None) | |
fromDict (cls, dictionary) | |
toDict (self) | |
fromTable (cls, tableList) | |
toTable (self) | |
subtractCrosstalk (self, thisExposure, sourceExposure=None, crosstalkCoeffs=None, crosstalkCoeffsSqr=None, crosstalkCoeffsValid=None, badPixels=["BAD"], minPixelToMask=45000, doSubtrahendMasking=False, crosstalkStr="CROSSTALK", isTrimmed=None, backgroundMethod="None", doSqrCrosstalk=False, fullAmplifier=False, parallelOverscan=None, detectorConfig=None, badAmpDict=None, ignoreVariance=False) | |
requiredAttributes (self) | |
requiredAttributes (self, value) | |
__str__ (self) | |
__eq__ (self, other) | |
metadata (self) | |
getMetadata (self) | |
setMetadata (self, metadata) | |
updateMetadataFromExposures (self, exposures) | |
calibInfoFromDict (self, dictionary) | |
determineCalibClass (cls, metadata, message) | |
readText (cls, filename, **kwargs) | |
writeText (self, filename, format="auto") | |
readFits (cls, filename, **kwargs) | |
writeFits (self, filename) | |
validate (self, other=None) | |
apply (self, target) | |
Static Public Member Functions | |
extractAmp (image, ampToFlip, ampTarget, isTrimmed=False, fullAmplifier=False, parallelOverscan=None) | |
calculateBackground (mi, badPixels=["BAD"]) | |
Public Attributes | |
bool | hasCrosstalk = False |
int | nAmp = nAmp if nAmp else 0 |
tuple | crosstalkShape = (self.nAmp, self.nAmp) |
int | coeffs = np.zeros(self.crosstalkShape) if self.nAmp else None |
int | coeffErr = np.zeros(self.crosstalkShape) if self.nAmp else None |
int | coeffNum |
int | coeffValid |
int | coeffsSqr = np.zeros(self.crosstalkShape) if self.nAmp else None |
int | coeffErrSqr = np.zeros(self.crosstalkShape) if self.nAmp else None |
int | ampGainRatios = np.zeros(self.crosstalkShape) if self.nAmp else None |
int | fitGains = np.zeros(self.nAmp) if self.nAmp else None |
str | crosstalkRatiosUnits = 'adu' if self.nAmp else None |
dict | interChip = {} |
requiredAttributes = set(["_OBSTYPE", "_SCHEMA", "_VERSION"]) | |
log = log if log else logging.getLogger(__name__) | |
Static Protected Member Functions | |
_getAppropriateBBox (amp, isTrimmed, fullAmplifier) | |
Protected Attributes | |
_instrument = None | |
_raftName = None | |
_slotName = None | |
_detectorName = None | |
_detectorSerial = None | |
_detectorId = None | |
_filter = None | |
str | _calibId = None |
_seqfile = None | |
_seqname = None | |
_seqcksum = None | |
_metadata = PropertyList() | |
_requiredAttributes | |
Static Protected Attributes | |
str | _OBSTYPE = "generic" |
str | _SCHEMA = "NO SCHEMA" |
int | _VERSION = 0 |
Calibration of amp-to-amp crosstalk coefficients. Parameters ---------- detector : `lsst.afw.cameraGeom.Detector`, optional Detector to use to pull coefficients from. nAmp : `int`, optional Number of amplifiers to initialize. log : `logging.Logger`, optional Log to write messages to. **kwargs : Parameters to pass to parent constructor. Notes ----- The crosstalk attributes stored are: hasCrosstalk : `bool` Whether there is crosstalk defined for this detector. nAmp : `int` Number of amplifiers in this detector. crosstalkShape : `tuple` [`int`, `int`] A tuple containing the shape of the ``coeffs`` matrix. This should be equivalent to (``nAmp``, ``nAmp``). coeffs : `numpy.ndarray` A matrix containing the crosstalk coefficients. coeff[i][j] contains the coefficients to calculate the contribution amplifier_j has on amplifier_i (each row[i] contains the corrections for detector_i). coeffErr : `numpy.ndarray`, optional A matrix (as defined by ``coeffs``) containing the standard distribution of the crosstalk measurements. coeffNum : `numpy.ndarray`, optional A matrix containing the number of pixel pairs used to measure the ``coeffs`` and ``coeffErr``. coeffValid : `numpy.ndarray`, optional A matrix of Boolean values indicating if the coefficient is valid, defined as abs(coeff) > coeffErr / sqrt(coeffNum). coeffsSqr : `numpy.ndarray`, optional A matrix containing potential quadratic crosstalk coefficients (see e.g., Snyder+21, 2001.03223). coeffsSqr[i][j] contains the coefficients to calculate the contribution amplifier_j has on amplifier_i (each row[i] contains the corrections for detector_i). coeffErrSqr : `numpy.ndarray`, optional A matrix (as defined by ``coeffsSqr``) containing the standard distribution of the quadratic term of the crosstalk measurements. interChip : `dict` [`numpy.ndarray`] A dictionary keyed by detectorName containing ``coeffs`` matrices used to correct for inter-chip crosstalk with a source on the detector indicated. Version 1.1 adds quadratic coefficients, a matrix with the ratios of amplifiers gains per detector, and a field to indicate the units of the numerator and denominator of the source and target signals, with "adu" meaning "ADU / ADU" and "electron" meaning "e- / e-". Version 1.2 adds the original gains used in the crosstalk fit.
Definition at line 43 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.__init__ | ( | self, | |
detector = None, | |||
nAmp = 0, | |||
** | kwargs ) |
Definition at line 107 of file crosstalk.py.
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Calibration equivalence. Running ``calib.log.setLevel(0)`` enables debug statements to identify problematic fields.
Definition at line 103 of file calibType.py.
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Definition at line 100 of file calibType.py.
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Get the appropriate bounding box from an amplifier. Parameters ---------- amp : `lsst.afw.cameraGeom.Amplifier` Amplifier to get bounding box. isTrimmed : `bool` Is this a trimmed image? fullAmplifier : `bool` Extract full amplifier for an untrimmed image?
Definition at line 544 of file crosstalk.py.
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Method to apply the calibration to the target object. Parameters ---------- target : `object` Thing to validate against. Returns ------- valid : `bool` Returns true if the calibration was applied correctly. Raises ------ NotImplementedError Raised if not implemented.
Definition at line 685 of file calibType.py.
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Estimate 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 564 of file crosstalk.py.
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Handle common keywords. This isn't an ideal solution, but until all calibrations expect to find everything in the metadata, they still need to search through dictionaries. Parameters ---------- dictionary : `dict` or `lsst.daf.base.PropertyList` Source for the common keywords. Raises ------ RuntimeError Raised if the dictionary does not match the expected OBSTYPE.
Definition at line 322 of file calibType.py.
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Attempt to find calibration class in metadata. Parameters ---------- metadata : `dict` or `lsst.daf.base.PropertyList` Metadata possibly containing a calibration class entry. message : `str` Message to include in any errors. Returns ------- calibClass : `object` The class to use to read the file contents. Should be an `lsst.ip.isr.IsrCalib` subclass. Raises ------ ValueError Raised if the resulting calibClass is the base `lsst.ip.isr.IsrClass` (which does not implement the content methods).
Definition at line 388 of file calibType.py.
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Extract the image data from an amp, flipped to match ampTarget. Parameters ---------- image : `lsst.afw.image.Image` or `lsst.afw.image.MaskedImage` Image containing the amplifier of interest. amp : `lsst.afw.cameraGeom.Amplifier` Amplifier on image to extract. ampTarget : `lsst.afw.cameraGeom.Amplifier` Target amplifier that the extracted image will be flipped to match. isTrimmed : `bool`, optional The image is already trimmed. fullAmplifier : `bool`, optional Use full amplifier and not just imaging region. parallelOverscan : `bool`, optional This has been deprecated and is unused, and will be removed after v29. Returns ------- output : `lsst.afw.image.Image` Amplifier from image, flipped to desired configuration. This will always return a copy of the original data.
Definition at line 489 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.fromDetector | ( | self, | |
detector, | |||
coeffVector = None, | |||
coeffSqrVector = None ) |
Set calibration parameters from the detector. Parameters ---------- detector : `lsst.afw.cameraGeom.Detector` Detector to use to set parameters from. coeffVector : `numpy.array`, optional Use the detector geometry (bounding boxes and flip information), but use ``coeffVector`` instead of the output of ``detector.getCrosstalk()``. coeffSqrVector : `numpy.array`, optional Quadratic crosstalk coefficients. Returns ------- calib : `lsst.ip.isr.CrosstalkCalib` The calibration constructed from the detector.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 167 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.fromDict | ( | cls, | |
dictionary ) |
Construct a calibration from a dictionary of properties. Must be implemented by the specific calibration subclasses. Parameters ---------- dictionary : `dict` Dictionary of properties. Returns ------- calib : `lsst.ip.isr.CalibType` Constructed calibration. Raises ------ RuntimeError Raised if the supplied dictionary is for a different calibration.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 226 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.fromTable | ( | cls, | |
tableList ) |
Construct calibration from a list of tables. This method uses the `fromDict` method to create the calibration, after constructing an appropriate dictionary from the input tables. Parameters ---------- tableList : `list` [`lsst.afw.table.Table`] List of tables to use to construct the crosstalk calibration. Returns ------- calib : `lsst.ip.isr.CrosstalkCalib` The calibration defined in the tables.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 393 of file crosstalk.py.
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Retrieve metadata associated with this calibration. Returns ------- meta : `lsst.daf.base.PropertyList` Metadata. The returned `~lsst.daf.base.PropertyList` can be modified by the caller and the changes will be written to external files.
Definition at line 171 of file calibType.py.
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Definition at line 168 of file calibType.py.
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Read calibration data from a FITS file. Parameters ---------- filename : `str` Filename to read data from. kwargs : `dict` or collections.abc.Mapping`, optional Set of key=value pairs to pass to the ``fromTable`` method. Returns ------- calib : `lsst.ip.isr.IsrCalib` Calibration contained within the file.
Definition at line 505 of file calibType.py.
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Read calibration representation from a yaml/ecsv file. Parameters ---------- filename : `str` Name of the file containing the calibration definition. kwargs : `dict` or collections.abc.Mapping`, optional Set of key=value pairs to pass to the ``fromDict`` or ``fromTable`` methods. Returns ------- calib : `~lsst.ip.isr.IsrCalibType` Calibration class. Raises ------ RuntimeError Raised if the filename does not end in ".ecsv" or ".yaml".
Definition at line 418 of file calibType.py.
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Definition at line 159 of file calibType.py.
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Definition at line 163 of file calibType.py.
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Store a copy of the supplied metadata with this calibration. Parameters ---------- metadata : `lsst.daf.base.PropertyList` Metadata to associate with the calibration. Will be copied and overwrite existing metadata.
Reimplemented in lsst.ip.isr.transmissionCurve.IntermediateTransmissionCurve.
Definition at line 183 of file calibType.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.subtractCrosstalk | ( | self, | |
thisExposure, | |||
sourceExposure = None, | |||
crosstalkCoeffs = None, | |||
crosstalkCoeffsSqr = None, | |||
crosstalkCoeffsValid = None, | |||
badPixels = ["BAD"], | |||
minPixelToMask = 45000, | |||
doSubtrahendMasking = False, | |||
crosstalkStr = "CROSSTALK", | |||
isTrimmed = None, | |||
backgroundMethod = "None", | |||
doSqrCrosstalk = False, | |||
fullAmplifier = False, | |||
parallelOverscan = None, | |||
detectorConfig = None, | |||
badAmpDict = None, | |||
ignoreVariance = False ) |
Subtract the crosstalk from thisExposure, optionally using a different source. We set the mask plane indicated by ``crosstalkStr`` in a target amplifier for pixels in a source amplifier that exceed ``minPixelToMask``, if ``doSubtrahendMasking`` is False. With that enabled, the mask is only set if the absolute value of the correction applied exceeds ``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 ---------- thisExposure : `lsst.afw.image.Exposure` Exposure for which to subtract crosstalk. sourceExposure : `lsst.afw.image.Exposure`, optional Exposure to use as the source of the crosstalk. If not set, thisExposure is used as the source (intra-detector crosstalk). crosstalkCoeffs : `numpy.ndarray`, optional. Coefficients to use to correct crosstalk. crosstalkCoeffsSqr : `numpy.ndarray`, optional. Quadratic coefficients to use to correct crosstalk. crosstalkCoeffsValid : `numpy.ndarray`, optional Boolean array that is True where coefficients are valid. badPixels : `list` of `str`, optional Mask planes to ignore. minPixelToMask : `float`, optional Minimum pixel value to set the ``crosstalkStr`` mask plane. If doSubtrahendMasking is True, this is calculated from the absolute magnitude of the subtrahend image. Otherwise, this sets the minimum source value to use to set that mask. doSubtrahendMasking : `bool`, optional If true, the mask is calculated from the properties of the subtrahend image, not from the brightness of the source pixel. crosstalkStr : `str`, optional Mask plane name for pixels greatly modified by crosstalk (above minPixelToMask). isTrimmed : `bool`, optional This option has been deprecated and does not do anything. It will be removed after v29. backgroundMethod : `str`, optional Method used to subtract the background. "AMP" uses amplifier-by-amplifier background levels, "DETECTOR" uses full exposure/maskedImage levels. Any other value results in no background subtraction. doSqrCrosstalk: `bool`, optional Should the quadratic crosstalk coefficients be used for the crosstalk correction? fullAmplifier : `bool`, optional Use full amplifier and not just imaging region. parallelOverscan : `bool`, optional This option is deprecated and will be removed after v29. detectorConfig : `lsst.ip.isr.overscanDetectorConfig`, optional Per-amplifier configs to use if parallelOverscan is True. This option is deprecated and will be removed after v29. badAmpDict : `dict` [`str`, `bool`], optional Dictionary to identify bad amplifiers that should not be source or target for crosstalk correction. ignoreVariance : `bool`, optional Ignore the variance plane when doing crosstalk correction? Notes ----- For a given image I, we want to find the crosstalk subtrahend image CT, such that I_corrected = I - CT The subtrahend image is the sum of all crosstalk contributions that appear in I, so we can build it up by amplifier. Each amplifier A in image I sees the contributions from all other amplifiers B_v != A. For the current linear model, we set `sImage` equal to the segment of the subtrahend image CT corresponding to amplifier A, and then build it up as: simage_linear = sum_v coeffsA_v * (B_v - bkg_v) where coeffsA_v is the vector of crosstalk coefficients for sources that cause images in amplifier A. The bkg_v term in this equation is identically 0.0 for all cameras except obs_subaru (and is only non-zero there for historical reasons). To include the non-linear term, we can again add to the subtrahend image using the same loop, as: simage_nonlinear = sum_v (coeffsA_v * B_v) + (NLcoeffsA_v * B_v * B_v) = sum_v linear_term_v + nonlinear_term_v where coeffsA_v is the linear term, and NLcoeffsA_v are the quadratic component. For LSSTCam, it has been observed that the linear_term_v >> nonlinear_term_v.
Definition at line 587 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.toDict | ( | self | ) |
Return a dictionary containing the calibration properties. The dictionary should be able to be round-tripped through `fromDict`. Returns ------- dictionary : `dict` Dictionary of properties.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 345 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.toTable | ( | self | ) |
Construct a list of tables containing the information in this calibration. The list of tables should create an identical calibration after being passed to this class's fromTable method. Returns ------- tableList : `list` [`lsst.afw.table.Table`] List of tables containing the crosstalk calibration information.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 448 of file crosstalk.py.
lsst.ip.isr.crosstalk.CrosstalkCalib.updateMetadata | ( | self, | |
setDate = False, | |||
** | kwargs ) |
Update calibration metadata. This calls the base class's method after ensuring the required calibration keywords will be saved. Parameters ---------- setDate : `bool`, optional Update the CALIBDATE fields in the metadata to the current time. Defaults to False. kwargs : Other keyword parameters to set in the metadata.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 142 of file crosstalk.py.
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Extract and unify metadata information. Parameters ---------- exposures : `list` Exposures or other calibrations to scan.
Definition at line 291 of file calibType.py.
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Validate that this calibration is defined and can be used. Parameters ---------- other : `object`, optional Thing to validate against. Returns ------- valid : `bool` Returns true if the calibration is valid and appropriate.
Reimplemented in lsst.ip.isr.linearize.Linearizer, and lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.
Definition at line 670 of file calibType.py.
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Write calibration data to a FITS file. Parameters ---------- filename : `str` Filename to write data to. Returns ------- used : `str` The name of the file used to write the data.
Reimplemented in lsst.ip.isr.transmissionCurve.IntermediateTransmissionCurve.
Definition at line 544 of file calibType.py.
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Write the calibration data to a text file. Parameters ---------- filename : `str` Name of the file to write. format : `str` Format to write the file as. Supported values are: ``"auto"`` : Determine filetype from filename. ``"yaml"`` : Write as yaml. ``"ecsv"`` : Write as ecsv. Returns ------- used : `str` The name of the file used to write the data. This may differ from the input if the format is explicitly chosen. Raises ------ RuntimeError Raised if filename does not end in a known extension, or if all information cannot be written. Notes ----- The file is written to YAML/ECSV format and will include any associated metadata.
Definition at line 451 of file calibType.py.
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Definition at line 74 of file calibType.py.
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Definition at line 72 of file calibType.py.
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Definition at line 70 of file calibType.py.
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Definition at line 71 of file calibType.py.
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Definition at line 73 of file calibType.py.
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Definition at line 67 of file calibType.py.
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Definition at line 78 of file calibType.py.
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Definition at line 62 of file calibType.py.
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Definition at line 68 of file calibType.py.
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Definition at line 113 of file calibType.py.
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Definition at line 63 of file calibType.py.
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Definition at line 77 of file calibType.py.
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Definition at line 75 of file calibType.py.
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Definition at line 76 of file calibType.py.
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Definition at line 69 of file calibType.py.
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Definition at line 64 of file calibType.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.ampGainRatios = np.zeros(self.crosstalkShape) if self.nAmp else None |
Definition at line 123 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.coeffErr = np.zeros(self.crosstalkShape) if self.nAmp else None |
Definition at line 113 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.coeffErrSqr = np.zeros(self.crosstalkShape) if self.nAmp else None |
Definition at line 120 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.coeffNum |
Definition at line 114 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.coeffs = np.zeros(self.crosstalkShape) if self.nAmp else None |
Definition at line 112 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.coeffsSqr = np.zeros(self.crosstalkShape) if self.nAmp else None |
Definition at line 119 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.coeffValid |
Definition at line 116 of file crosstalk.py.
str lsst.ip.isr.crosstalk.CrosstalkCalib.crosstalkRatiosUnits = 'adu' if self.nAmp else None |
Definition at line 129 of file crosstalk.py.
tuple lsst.ip.isr.crosstalk.CrosstalkCalib.crosstalkShape = (self.nAmp, self.nAmp) |
Definition at line 110 of file crosstalk.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.fitGains = np.zeros(self.nAmp) if self.nAmp else None |
Definition at line 126 of file crosstalk.py.
bool lsst.ip.isr.crosstalk.CrosstalkCalib.hasCrosstalk = False |
Definition at line 108 of file crosstalk.py.
dict lsst.ip.isr.crosstalk.CrosstalkCalib.interChip = {} |
Definition at line 131 of file crosstalk.py.
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Definition at line 94 of file calibType.py.
int lsst.ip.isr.crosstalk.CrosstalkCalib.nAmp = nAmp if nAmp else 0 |
Definition at line 109 of file crosstalk.py.
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Definition at line 88 of file calibType.py.