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
Public Member Functions | List of all members
lsst.obs.test.testCamera.TestCamera Class Reference
Inheritance diagram for lsst.obs.test.testCamera.TestCamera:

Public Member Functions

def __new__ (cls)
 
def __init__ (self)
 

Detailed Description

A simple test Camera.

Notes
-----
The camera has one ccd with name "0".
That CCD has four amplifiers with names "00", "01", "10", and "11".

The camera is modeled after a small portion of the LSST sim
Summer 2012 camera: a single detector with four amplifiers,
consisting of raft 2,2 sensor 0,0, half of channels 0,0 0,1 1,0 and 1,1
(the half closest to the Y centerline).

Note that the Summer 2012 camera has one very weird feature:
the bias region (rawHOverscanBbox) is actually a prescan
(it appears before the data pixels).

A raw image has the sky in the same orientation on all amplifier
subregions, so no amplifier subregions need their pixels to be flipped.

Standard keys are:

* ``amp``: amplifier number: one of 00, 01, 10, 11
* ``ccd``: ccd number: always 0
* ``visit``: exposure number; test data includes one exposure
    with visit=1

Definition at line 31 of file testCamera.py.

Constructor & Destructor Documentation

◆ __init__()

def lsst.obs.test.testCamera.TestCamera.__init__ (   self)

Definition at line 75 of file testCamera.py.

75  def __init__(self):
76  pass
77 

Member Function Documentation

◆ __new__()

def lsst.obs.test.testCamera.TestCamera.__new__ (   cls)

Definition at line 58 of file testCamera.py.

58  def __new__(cls):
59  plateScale = geom.Angle(20, geom.arcseconds) # plate scale, in angle on sky/mm
60  # Radial distortion is modeled as a radial polynomial that converts from focal plane (in mm)
61  # to field angle (in radians). Thus the coefficients are:
62  # C0: always 0, for continuity at the center of the focal plane; units are rad
63  # C1: 1/plateScale; units are rad/mm
64  # C2: usually 0; units are rad/mm^2
65  # C3: radial distortion; units are rad/mm^3
66  radialCoeff = np.array([0.0, 1.0, 0.0, 0.925]) / plateScale.asRadians()
67  fieldAngleToFocalPlane = afwGeom.makeRadialTransform(radialCoeff)
68  focalPlaneToFieldAngle = fieldAngleToFocalPlane.inverted()
69 
70  camera = cameraGeom.Camera.Builder("test")
71  cls._makeDetectors(camera, focalPlaneToFieldAngle)
72  camera.setTransformFromFocalPlaneTo(cameraGeom.FIELD_ANGLE, focalPlaneToFieldAngle)
73  return camera.finish()
74 
A class representing an angle.
Definition: Angle.h:127
std::shared_ptr< TransformPoint2ToPoint2 > makeRadialTransform(std::vector< double > const &coeffs)
A purely radial polynomial distortion.

The documentation for this class was generated from the following file: