LSST Applications  21.0.0+04719a4bac,21.0.0-1-ga51b5d4+f5e6047307,21.0.0-11-g2b59f77+a9c1acf22d,21.0.0-11-ga42c5b2+86977b0b17,21.0.0-12-gf4ce030+76814010d2,21.0.0-13-g1721dae+760e7a6536,21.0.0-13-g3a573fe+768d78a30a,21.0.0-15-g5a7caf0+f21cbc5713,21.0.0-16-g0fb55c1+b60e2d390c,21.0.0-19-g4cded4ca+71a93a33c0,21.0.0-2-g103fe59+bb20972958,21.0.0-2-g45278ab+04719a4bac,21.0.0-2-g5242d73+3ad5d60fb1,21.0.0-2-g7f82c8f+8babb168e8,21.0.0-2-g8f08a60+06509c8b61,21.0.0-2-g8faa9b5+616205b9df,21.0.0-2-ga326454+8babb168e8,21.0.0-2-gde069b7+5e4aea9c2f,21.0.0-2-gecfae73+1d3a86e577,21.0.0-2-gfc62afb+3ad5d60fb1,21.0.0-25-g1d57be3cd+e73869a214,21.0.0-3-g357aad2+ed88757d29,21.0.0-3-g4a4ce7f+3ad5d60fb1,21.0.0-3-g4be5c26+3ad5d60fb1,21.0.0-3-g65f322c+e0b24896a3,21.0.0-3-g7d9da8d+616205b9df,21.0.0-3-ge02ed75+a9c1acf22d,21.0.0-4-g591bb35+a9c1acf22d,21.0.0-4-g65b4814+b60e2d390c,21.0.0-4-gccdca77+0de219a2bc,21.0.0-4-ge8a399c+6c55c39e83,21.0.0-5-gd00fb1e+05fce91b99,21.0.0-6-gc675373+3ad5d60fb1,21.0.0-64-g1122c245+4fb2b8f86e,21.0.0-7-g04766d7+cd19d05db2,21.0.0-7-gdf92d54+04719a4bac,21.0.0-8-g5674e7b+d1bd76f71f,master-gac4afde19b+a9c1acf22d,w.2021.13
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:746
A base class for image defects.