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Proceedings Paper

Characterization of LSST CCDs using realistic images, before first light
Author(s): Andrew K. Bradshaw; Craig Lage; J. Anthony Tyson
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Paper Abstract

The 3.2 gigapixel LSST camera, an array of 189 thick fully-depleted CCDs, will repeatedly image the southern sky and accomplish a wide variety of science goals. However, its trove of tens of billions of object images implies stringent requirements on systematic biases imprinted during shift-and-stare CCD observation. In order to correct for these biases which, without correction, violate requirements on weak lensing precision, we investigate CCD systematics using both simulations of charge transport as well as with a unique bench-top optical system matched to the LSST’s fast f/1.2 beam. By illuminating single CCDs with realistic scenes of stars and galaxies and then analyzing these images with the LSST data management pipelines, we can characterize the survey’s imaging performance well before the camera’s first light. We present measurements of several CCD systematics under varying conditions in the laboratory, including the brightness-dependent broadening of star and galaxy images, charge transport anomalies in the silicon bulk as well as the edges, and serial deferred charge. Alongside these measurements, we also present the development and testing of physics-based models which inform corrections or mitigation strategies for these systematics. Optimization of the CCD survey operation under a variety of realistic observational conditions, including systematic effects from the optics, clocking, sky brightness, and image analysis, will be critical to achieve the LSST’s goals of precision astronomy and cosmology.

Paper Details

Date Published: 12 July 2018
PDF: 13 pages
Proc. SPIE 10709, High Energy, Optical, and Infrared Detectors for Astronomy VIII, 107091L (12 July 2018); doi: 10.1117/12.2314276
Show Author Affiliations
Andrew K. Bradshaw, Univ. of California, Davis (United States)
Craig Lage, Univ. of California, Davis (United States)
J. Anthony Tyson, Univ. of California, Davis (United States)

Published in SPIE Proceedings Vol. 10709:
High Energy, Optical, and Infrared Detectors for Astronomy VIII
Andrew D. Holland; James Beletic, Editor(s)

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