LSSTApplications
18.0.0+106,18.0.0+50,19.0.0,19.0.0+1,19.0.0+10,19.0.0+11,19.0.0+13,19.0.0+17,19.0.0+2,19.0.0-1-g20d9b18+6,19.0.0-1-g425ff20,19.0.0-1-g5549ca4,19.0.0-1-g580fafe+6,19.0.0-1-g6fe20d0+1,19.0.0-1-g7011481+9,19.0.0-1-g8c57eb9+6,19.0.0-1-gb5175dc+11,19.0.0-1-gdc0e4a7+9,19.0.0-1-ge272bc4+6,19.0.0-1-ge3aa853,19.0.0-10-g448f008b,19.0.0-12-g6990b2c,19.0.0-2-g0d9f9cd+11,19.0.0-2-g3d9e4fb2+11,19.0.0-2-g5037de4,19.0.0-2-gb96a1c4+3,19.0.0-2-gd955cfd+15,19.0.0-3-g2d13df8,19.0.0-3-g6f3c7dc,19.0.0-4-g725f80e+11,19.0.0-4-ga671dab3b+1,19.0.0-4-gad373c5+3,19.0.0-5-ga2acb9c+2,19.0.0-5-gfe96e6c+2,w.2020.01
LSSTDataManagementBasePackage
|
Classes | |
class | SkyMapIdContainer |
Functions | |
def | cropFakeImage (fakeImage, expBBox) |
def | addNoise (galImage, detector, rand_gen=None) |
def lsst.synpipe.FakeSourceLib.addNoise | ( | galImage, | |
detector, | |||
rand_gen = None |
|||
) |
adds noise to the the image and returns a variance plane INPUT: image to add noise to detector where the image will be located, this sets the gain NOTE: this assumes float type images and will break if given doubles RETURN: a MaskedImageF with the image with additional noise and the variance plane giving the variance due to the object
Definition at line 63 of file FakeSourceLib.py.
def lsst.synpipe.FakeSourceLib.cropFakeImage | ( | fakeImage, | |
expBBox | |||
) |
Crops the Fake image to fit inside the exposure BBox Note that the bboxes need to have the correct offsets applied Args: fakeImage: fake image object expBBox: bounding box for CCD exposure (integer type, BBoxI) and with offsets applied Returns: New cropped fake image
Definition at line 41 of file FakeSourceLib.py.