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LSST Data Management Base Package
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Public Member Functions | |
__eq__ (self, other) | |
fromTable (cls, table) | |
toTable (self) | |
evaluate (self, detector, position, wavelength, kind='linear', bounds_error=False, fill_value=0) | |
Public Attributes | |
wavelength | |
efficiency | |
Static Public Attributes | |
str | mode = 'DETECTOR' |
Subclass of `Curve` that represents a single curve per detector. Parameters ---------- wavelength : `astropy.units.Quantity` Wavelength values for this curve efficiency : `astropy.units.Quantity` Quantum efficiency values for this curve metadata : `dict` Dictionary of metadata for this curve
Definition at line 296 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.DetectorCurve.__eq__ | ( | self, | |
other ) |
Define equality for this class
Reimplemented from lsst.meas.algorithms.simple_curve.Curve.
Definition at line 310 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.DetectorCurve.evaluate | ( | self, | |
detector, | |||
position, | |||
wavelength, | |||
kind = 'linear', | |||
bounds_error = False, | |||
fill_value = 0 ) |
Interpolate the curve at the specified position and wavelength. Parameters ---------- detector : `lsst.afw.cameraGeom.Detector` Is used to find the appropriate curve given the position for curves that vary over the detector. Ignored in the case where there is only a single curve per detector. position : `lsst.geom.Point2D` The position on the detector at which to evaluate the curve. wavelength : `astropy.units.Quantity` The wavelength(s) at which to make the interpolation. kind : `str`, optional The type of interpolation to do (default is 'linear'). See documentation for `scipy.interpolate.interp1d` for accepted values. bounds_error : `bool`, optional Raise error if interpolating outside the range of x? (default is False) fill_value : `float`, optional Fill values outside the range of x with this value (default is 0). Returns ------- value : `astropy.units.Quantity` Interpolated value(s). Number of values returned will match the length of `wavelength`. Raises ------ ValueError If the ``bounds_error`` is changed from the default, it will raise a `ValueError` if evaluating outside the bounds of the curve.
Reimplemented from lsst.meas.algorithms.simple_curve.Curve.
Definition at line 325 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.DetectorCurve.fromTable | ( | cls, | |
table ) |
Class method for constructing a `Curve` object. Parameters ---------- table : `astropy.table.QTable` Table containing metadata and columns necessary for constructing a `Curve` object. Returns ------- curve : `Curve` A `Curve` subclass of the appropriate type according to the table metadata
Reimplemented from lsst.meas.algorithms.simple_curve.Curve.
Definition at line 316 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.DetectorCurve.toTable | ( | self | ) |
Convert this `Curve` object to an `astropy.table.QTable`. Returns ------- table : `astropy.table.QTable` A table object containing the data from this `Curve`.
Reimplemented from lsst.meas.algorithms.simple_curve.Curve.
Definition at line 321 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.DetectorCurve.efficiency |
Definition at line 327 of file simple_curve.py.
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static |
Definition at line 308 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.DetectorCurve.wavelength |
Definition at line 312 of file simple_curve.py.