LSST Applications
21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
LSST Data Management Base Package
|
Public Member Functions | |
def | __init__ (self, amp_name_list, wavelength, efficiency, metadata) |
def | __eq__ (self, other) |
def | fromTable (cls, table) |
def | toTable (self) |
def | evaluate (self, detector, position, wavelength, kind='linear', bounds_error=False, fill_value=0) |
def | __init_subclass__ (cls, **kwargs) |
def | compare_metadata (self, other, keys_to_compare=['MODE', 'TYPE', 'CALIBDATE', 'INSTRUME', 'OBSTYPE', 'DETECTOR']) |
def | interpolate (self, wavelengths, values, wavelength, kind, bounds_error, fill_value) |
def | getMetadata (self) |
def | readText (cls, filename) |
def | readFits (cls, filename) |
def | writeText (self, filename) |
def | writeFits (self, filename) |
Public Attributes | |
data | |
wavelength | |
efficiency | |
metadata | |
Static Public Attributes | |
string | mode = 'AMP' |
subclasses = dict() | |
Subclass of `Curve` that represents a curve per amp. Parameters ---------- amp_name_list : iterable of `str` The name of the amp for each entry 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 331 of file simple_curve.py.
def lsst.meas.algorithms.simple_curve.AmpCurve.__init__ | ( | self, | |
amp_name_list, | |||
wavelength, | |||
efficiency, | |||
metadata | |||
) |
Definition at line 347 of file simple_curve.py.
def lsst.meas.algorithms.simple_curve.AmpCurve.__eq__ | ( | self, | |
other | |||
) |
Define equality for this class
Reimplemented from lsst.meas.algorithms.simple_curve.Curve.
Definition at line 359 of file simple_curve.py.
|
inherited |
Register subclasses with the abstract base class
Definition at line 126 of file simple_curve.py.
|
inherited |
Compare metadata in this object to another. Parameters ---------- other : `Curve` The object with which to compare metadata. keys_to_compare : `list` List of metadata keys to compare. Returns ------- same : `bool` Are the metadata the same?
Definition at line 138 of file simple_curve.py.
def lsst.meas.algorithms.simple_curve.AmpCurve.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 401 of file simple_curve.py.
def lsst.meas.algorithms.simple_curve.AmpCurve.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 370 of file simple_curve.py.
|
inherited |
Return metadata Returns ------- metadata : `dict` Dictionary of metadata for this curve.
Definition at line 187 of file simple_curve.py.
|
inherited |
Interplate the curve at the specified wavelength(s). Parameters ---------- wavelengths : `astropy.units.Quantity` The wavelength values for the curve. values : `astropy.units.Quantity` The y-values for the curve. wavelength : `astropy.units.Quantity` The wavelength(s) at which to make the interpolation. kind : `str` The type of interpolation to do. See documentation for `scipy.interpolate.interp1d` for accepted values. Returns ------- value : `astropy.units.Quantity` Interpolated value(s)
Definition at line 159 of file simple_curve.py.
|
inherited |
Class method for constructing a `Curve` object from the standardized FITS format. Parameters ---------- filename : `str` Path to the FITS file to read. Returns ------- curve : `Curve` A `Curve` subclass of the appropriate type according to the table metadata
Definition at line 218 of file simple_curve.py.
|
inherited |
Class method for constructing a `Curve` object from the standardized text format. Parameters ---------- filename : `str` Path to the text file to read. Returns ------- curve : `Curve` A `Curve` subclass of the appropriate type according to the table metadata
Definition at line 199 of file simple_curve.py.
def lsst.meas.algorithms.simple_curve.AmpCurve.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 376 of file simple_curve.py.
|
inherited |
Write the `Curve` out to a FITS file. Parameters ---------- filename : `str` Path to the FITS file to write. Returns ------- filename : `str` Because this method forces a particular extension return the name of the file actually written.
Definition at line 274 of file simple_curve.py.
|
inherited |
Write the `Curve` out to a text file. Parameters ---------- filename : `str` Path to the text file to write. Returns ------- filename : `str` Because this method forces a particular extension return the name of the file actually written.
Definition at line 253 of file simple_curve.py.
lsst.meas.algorithms.simple_curve.AmpCurve.data |
Definition at line 350 of file simple_curve.py.
|
inherited |
Definition at line 51 of file simple_curve.py.
|
inherited |
Definition at line 54 of file simple_curve.py.
|
static |
Definition at line 345 of file simple_curve.py.
|
staticinherited |
Definition at line 43 of file simple_curve.py.
|
inherited |
Definition at line 50 of file simple_curve.py.