LSST Applications
21.0.0-147-g0e635eb1+1acddb5be5,22.0.0+052faf71bd,22.0.0+1ea9a8b2b2,22.0.0+6312710a6c,22.0.0+729191ecac,22.0.0+7589c3a021,22.0.0+9f079a9461,22.0.1-1-g7d6de66+b8044ec9de,22.0.1-1-g87000a6+536b1ee016,22.0.1-1-g8e32f31+6312710a6c,22.0.1-10-gd060f87+016f7cdc03,22.0.1-12-g9c3108e+df145f6f68,22.0.1-16-g314fa6d+c825727ab8,22.0.1-19-g93a5c75+d23f2fb6d8,22.0.1-19-gb93eaa13+aab3ef7709,22.0.1-2-g8ef0a89+b8044ec9de,22.0.1-2-g92698f7+9f079a9461,22.0.1-2-ga9b0f51+052faf71bd,22.0.1-2-gac51dbf+052faf71bd,22.0.1-2-gb66926d+6312710a6c,22.0.1-2-gcb770ba+09e3807989,22.0.1-20-g32debb5+b8044ec9de,22.0.1-23-gc2439a9a+fb0756638e,22.0.1-3-g496fd5d+09117f784f,22.0.1-3-g59f966b+1e6ba2c031,22.0.1-3-g849a1b8+f8b568069f,22.0.1-3-gaaec9c0+c5c846a8b1,22.0.1-32-g5ddfab5d3+60ce4897b0,22.0.1-4-g037fbe1+64e601228d,22.0.1-4-g8623105+b8044ec9de,22.0.1-5-g096abc9+d18c45d440,22.0.1-5-g15c806e+57f5c03693,22.0.1-7-gba73697+57f5c03693,master-g6e05de7fdc+c1283a92b8,master-g72cdda8301+729191ecac,w.2021.39
LSST Data Management Base Package
|
Classes | |
class | DcrModel |
Functions | |
def | applyDcr (image, dcr, useInverse=False, splitSubfilters=False, splitThreshold=0., doPrefilter=True, order=3) |
def | calculateDcr (visitInfo, wcs, effectiveWavelength, bandwidth, dcrNumSubfilters, splitSubfilters=False) |
def | calculateImageParallacticAngle (visitInfo, wcs) |
def | wavelengthGenerator (effectiveWavelength, bandwidth, dcrNumSubfilters) |
def lsst.ip.diffim.dcrModel.applyDcr | ( | image, | |
dcr, | |||
useInverse = False , |
|||
splitSubfilters = False , |
|||
splitThreshold = 0. , |
|||
doPrefilter = True , |
|||
order = 3 |
|||
) |
Shift an image along the X and Y directions. Parameters ---------- image : `numpy.ndarray` The input image to shift. dcr : `tuple` Shift calculated with ``calculateDcr``. Uses numpy axes ordering (Y, X). If ``splitSubfilters`` is set, each element is itself a `tuple` of two `float`, corresponding to the DCR shift at the two wavelengths. Otherwise, each element is a `float` corresponding to the DCR shift at the effective wavelength of the subfilter. useInverse : `bool`, optional Apply the shift in the opposite direction. Default: False splitSubfilters : `bool`, optional Calculate DCR for two evenly-spaced wavelengths in each subfilter, instead of at the midpoint. Default: False splitThreshold : `float`, optional Minimum DCR difference within a subfilter required to use ``splitSubfilters`` doPrefilter : `bool`, optional Spline filter the image before shifting, if set. Filtering is required, so only set to False if the image is already filtered. Filtering takes ~20% of the time of shifting, so if `applyDcr` will be called repeatedly on the same image it is more efficient to precalculate the filter. order : `int`, optional The order of the spline interpolation, default is 3. Returns ------- shiftedImage : `numpy.ndarray` A copy of the input image with the specified shift applied.
Definition at line 693 of file dcrModel.py.
def lsst.ip.diffim.dcrModel.calculateDcr | ( | visitInfo, | |
wcs, | |||
effectiveWavelength, | |||
bandwidth, | |||
dcrNumSubfilters, | |||
splitSubfilters = False |
|||
) |
Calculate the shift in pixels of an exposure due to DCR. Parameters ---------- visitInfo : `lsst.afw.image.VisitInfo` Metadata for the exposure. wcs : `lsst.afw.geom.SkyWcs` Coordinate system definition (wcs) for the exposure. effectiveWavelength : `float` The effective wavelengths of the current filter, in nanometers. bandwidth : `float` The bandwidth of the current filter, in nanometers. dcrNumSubfilters : `int` Number of sub-filters used to model chromatic effects within a band. splitSubfilters : `bool`, optional Calculate DCR for two evenly-spaced wavelengths in each subfilter, instead of at the midpoint. Default: False Returns ------- dcrShift : `tuple` of two `float` The 2D shift due to DCR, in pixels. Uses numpy axes ordering (Y, X).
Definition at line 759 of file dcrModel.py.
def lsst.ip.diffim.dcrModel.calculateImageParallacticAngle | ( | visitInfo, | |
wcs | |||
) |
Calculate the total sky rotation angle of an exposure. Parameters ---------- visitInfo : `lsst.afw.image.VisitInfo` Metadata for the exposure. wcs : `lsst.afw.geom.SkyWcs` Coordinate system definition (wcs) for the exposure. Returns ------- `lsst.geom.Angle` The rotation of the image axis, East from North. Equal to the parallactic angle plus any additional rotation of the coordinate system. A rotation angle of 0 degrees is defined with North along the +y axis and East along the +x axis. A rotation angle of 90 degrees is defined with North along the +x axis and East along the -y axis.
Definition at line 815 of file dcrModel.py.
def lsst.ip.diffim.dcrModel.wavelengthGenerator | ( | effectiveWavelength, | |
bandwidth, | |||
dcrNumSubfilters | |||
) |
Iterate over the wavelength endpoints of subfilters. Parameters ---------- effectiveWavelength : `float` The effective wavelength of the current filter, in nanometers. bandwidth : `float` The bandwidth of the current filter, in nanometers. dcrNumSubfilters : `int` Number of sub-filters used to model chromatic effects within a band. Yields ------ `tuple` of two `float` The next set of wavelength endpoints for a subfilter, in nanometers.
Definition at line 847 of file dcrModel.py.