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
lsst::obs::test; Simple camera and data repository for testing

obs_test models a simple camera with one CCD and includes a data repository containing a few raw images and some associated calibration data.

obs_test is designed to be used for unit tests that require camera geometry and/or a small data repository.

Camera

The obs_test camera consists of a single CCD whose geometry matches a subregion of a single LSST CCD. The chosen LSST CCD is is near, but not at, the center of the LSST focal plane, in order to make the obs_test camera geometry nontrivial and to provide a bit of distortion. A subregion is used (rather than simply using an entire LSST CCD) in order to make the images smaller.

In detail, the obs_test CCD, sensor 0, corresponds to the following LSST CCD subregion:

  • Raft R2,2 (the center raft)
  • CCD/sensor S0,0 (the lower left CCD in the raft)
  • Amplifiers/channels C0,0, C0,1, C1,0 C1,1, keeping only the 1000 pixels in Y nearest the center line of the CCD

obs_test CCD amplifiers map as follows to LSST CCD amplifiers:

  • "00" = "C0,0"
  • "10" = "C0,1"
  • "01" = "C1,0"
  • "11" = "C1,1"

The data ID keys that may be used to identify "raw" images and (except for "amp") "calexp" images are:

  • amp: amplifier name: one of "00", "01", "10", "11" (not used for calexp)
  • ccd: ccd number: always 0
  • filter: filter name
  • visit: exposure number

Like the LSST camera, the obs_test camera focal plane coordinates are rotated 90 degrees from pixel coordinates. (The focal plane coordinates are determined by the camera engineers, whereas CCD pixel coordinates are required to have x along rows and y along columns).

Data

The data directory includes the following:

  • ReadMe.md: a file describing the data and how it was generated
  • input: the data repository. This includes three raw images and associated flats, biases and defects.
  • utils: scripts used to generate the data from lsstSim data

Unlike the LSST camera, but like most other cameras, obs_test raw images combine the data from all amplifiers into a single image.

Classes

Useful classes include:

  • TestCamera: camera geometry for the obs_test camera. Unlike most obs_* packages this package builds its own camera geometry (by instantiating this class), rather than relying on the lsst.obs.base.CameraMapper to load camera geometry data from a persisted lsst.afw.cameraGeom.CameraConfig.
  • TestMapper: camera mapper for the obs_test camera

Example

To obtain the camera geometry and a raw image:

import os.path
import lsst.utils
obsTestDir = lsst.utils.getPackageDir('obs_test')
input = os.path.join(obsTestDir, "data", "input")
butler = lsst.daf.persistence.Butler(root = input) # don't add to the input repo
rawImage = butler.get("raw", dict(visit=1))
cameraGeom = butler.get("camera")
std::ostream * os
Definition: Schema.cc:557
A base class for image defects.