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lsst.ip.isr g24cdac46ce+2390a8f09a
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Public Member Functions | |
| __init__ (self, table=None, **kwargs) | |
| fromDict (cls, dictionary) | |
| toDict (self) | |
| fromTable (cls, tableList) | |
| toTable (self) | |
| getIntrinsicZernikes (self, field_x, field_y, noll_indices=None) | |
| requiredAttributes (self) | |
| requiredAttributes (self, value) | |
| __str__ (self) | |
| __eq__ (self, other) | |
| metadata (self) | |
| getMetadata (self) | |
| setMetadata (self, metadata) | |
| updateMetadata (self, camera=None, detector=None, filterName=None, setCalibId=False, setCalibInfo=False, setDate=False, **kwargs) | |
| 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) | |
| fromDetector (self, detector) | |
| validate (self, other=None) | |
| apply (self, target) | |
Public Attributes | |
| field_x = np.array([]) | |
| field_y = np.array([]) | |
| values = np.array([]) | |
| noll_indices = np.array([]) | |
| interpolator = None | |
| requiredAttributes = set(["_OBSTYPE", "_SCHEMA", "_VERSION"]) | |
| log = log if log else logging.getLogger(__name__) | |
Protected Member Functions | |
| _createInterpolator (self) | |
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 |
Intrinsic Zernike coefficients.
Stores Zernike wavefront-error coefficients sampled at a set of
focal-plane field angles. At query time the coefficients are
interpolated to an arbitrary field position.
Field angles are expressed in the Camera Coordinate System (CCS), also
known as the Engineering Diagram Coordinate System. See
`LSE-349 <https://ls.st/LSE-349>`_ for the definition.
Parameters
----------
table : `astropy.table.Table`, optional
Source table. Must contain columns:
``"x"``
Field x positions (in CCS) with angular units (e.g. ``u.deg``).
``"y"``
Field y positions (in CCS) with angular units (e.g. ``u.deg``).
``"Z{j}"``
One column per Noll index *j*, with length units
(e.g. ``u.um``).
Attributes
----------
field_x : `numpy.ndarray`
CCS x field positions in degrees for all sample points,
shape ``(n_points,)``.
field_y : `numpy.ndarray`
CCS y field positions in degrees for all sample points,
shape ``(n_points,)``.
noll_indices : `numpy.ndarray`
Noll indices of the stored Zernike terms, shape ``(n_zernikes,)``.
values : `numpy.ndarray`
Zernike coefficients in microns, shape
``(n_points, n_zernikes)``.
interpolator : `scipy.interpolate.LinearNDInterpolator` or `None`
Interpolator built from ``field_x``, ``field_y``, and
``values``. ``None`` until the calibration is populated.
Definition at line 35 of file intrinsicZernikes.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.__init__ | ( | self, | |
| table = None, | |||
| ** | kwargs ) |
Definition at line 81 of file intrinsicZernikes.py.
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Calibration equivalence. Running ``calib.log.setLevel(0)`` enables debug statements to identify problematic fields.
Definition at line 105 of file calibType.py.
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inherited |
Definition at line 102 of file calibType.py.
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protected |
Definition at line 105 of file intrinsicZernikes.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 706 of file calibType.py.
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inherited |
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 325 of file calibType.py.
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inherited |
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 391 of file calibType.py.
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inherited |
Modify the calibration parameters to match the supplied detector.
Parameters
----------
detector : `lsst.afw.cameraGeom.Detector`
Detector to use to set parameters from.
Raises
------
NotImplementedError
Raised if not implemented by a subclass.
This needs to be implemented by subclasses for each
calibration type.
Reimplemented in lsst.ip.isr.crosstalk.CrosstalkCalib, lsst.ip.isr.deferredCharge.DeferredChargeCalib, lsst.ip.isr.linearize.Linearizer, and lsst.ip.isr.ptcDataset.PhotonTransferCurveDataset.
Definition at line 588 of file calibType.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.fromDict | ( | cls, | |
| dictionary ) |
Construct an IntrinsicZernikes from dictionary of properties.
Parameters
----------
dictionary : `dict`
Dictionary of properties.
Returns
-------
calib : `lsst.ip.isr.IntrinsicZernikes`
Constructed calibration.
Raises
------
RuntimeError
Raised if the supplied dictionary is for a different
calibration type.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 112 of file intrinsicZernikes.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.fromTable | ( | cls, | |
| tableList ) |
Construct calibration from a list of tables.
Parameters
----------
tableList : `list` [`astropy.table.Table`]
List of tables to use to construct the intrinsic zernikes
calibration.
Returns
-------
calib : `lsst.ip.isr.IntrinsicZernikes`
The calibration defined in the tables.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 172 of file intrinsicZernikes.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.getIntrinsicZernikes | ( | self, | |
| field_x, | |||
| field_y, | |||
| noll_indices = None ) |
Get the intrinsic Zernike coefficients at a given field position.
Parameters
----------
field_x : `array-like`
CCS x-field positions in degrees.
field_y : `array-like`
CCS y-field positions in degrees.
noll_indices : `list` [`int`], optional
List of Noll indices to return. If None, return all.
Returns
-------
zernikes : `array-like`
Array of Zernike coefficient values in microns corresponding to the
requested Noll indices and field positions.
Definition at line 223 of file intrinsicZernikes.py.
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inherited |
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 174 of file calibType.py.
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inherited |
Definition at line 171 of file calibType.py.
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inherited |
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 517 of file calibType.py.
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inherited |
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 425 of file calibType.py.
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inherited |
Definition at line 162 of file calibType.py.
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inherited |
Definition at line 166 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 186 of file calibType.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.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 149 of file intrinsicZernikes.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.toTable | ( | self | ) |
Construct a list of tables containing the information in this
calibration.
The list of tables should be able to be round-tripped through
`fromTable`.
Returns
-------
tableList : `list` [`astropy.table.Table`]
List of tables containing the intrinsic zernikes calibration
information.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 192 of file intrinsicZernikes.py.
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inherited |
Update metadata keywords with new values.
Parameters
----------
camera : `lsst.afw.cameraGeom.Camera`, optional
Reference camera to use to set ``_instrument`` field.
detector : `lsst.afw.cameraGeom.Detector`, optional
Reference detector to use to set ``_detector*`` fields.
filterName : `str`, optional
Filter name to assign to this calibration.
setCalibId : `bool`, optional
Construct the ``_calibId`` field from other fields.
setCalibInfo : `bool`, optional
Set calibration parameters from metadata.
setDate : `bool`, optional
Ensure the metadata ``CALIBDATE`` fields are set to the current
datetime.
kwargs : `dict` or `collections.abc.Mapping`, optional
Set of ``key=value`` pairs to assign to the metadata.
Reimplemented in lsst.ip.isr.brighterFatterKernel.BrighterFatterKernel, lsst.ip.isr.calibType.IsrProvenance, lsst.ip.isr.crosstalk.CrosstalkCalib, lsst.ip.isr.electrostaticBrighterFatter.ElectrostaticBrighterFatterDistortionMatrix, lsst.ip.isr.linearize.Linearizer, lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection, and lsst.ip.isr.ptcDataset.PhotonTransferCurveDataset.
Definition at line 208 of file calibType.py.
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inherited |
Extract and unify metadata information.
Parameters
----------
exposures : `list`
Exposures or other calibrations to scan.
Definition at line 294 of file calibType.py.
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inherited |
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 691 of file calibType.py.
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inherited |
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 565 of file calibType.py.
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inherited |
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 463 of file calibType.py.
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Definition at line 76 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 73 of file calibType.py.
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Definition at line 75 of file calibType.py.
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Definition at line 69 of file calibType.py.
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Definition at line 80 of file calibType.py.
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Definition at line 64 of file calibType.py.
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Definition at line 70 of file calibType.py.
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Definition at line 115 of file calibType.py.
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Definition at line 65 of file calibType.py.
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Definition at line 79 of file calibType.py.
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Definition at line 77 of file calibType.py.
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Definition at line 78 of file calibType.py.
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Definition at line 71 of file calibType.py.
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Definition at line 66 of file calibType.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.field_x = np.array([]) |
Definition at line 82 of file intrinsicZernikes.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.field_y = np.array([]) |
Definition at line 83 of file intrinsicZernikes.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.interpolator = None |
Definition at line 86 of file intrinsicZernikes.py.
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Definition at line 96 of file calibType.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.noll_indices = np.array([]) |
Definition at line 85 of file intrinsicZernikes.py.
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Definition at line 90 of file calibType.py.
| lsst.ip.isr.intrinsicZernikes.IntrinsicZernikes.values = np.array([]) |
Definition at line 84 of file intrinsicZernikes.py.