Presentation + Paper
12 July 2018 Characterization of LSST CCDs using realistic images, before first light
Andrew K. Bradshaw, Craig Lage, J. Anthony Tyson
Author Affiliations +
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.
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrew K. Bradshaw, Craig Lage, and J. Anthony Tyson "Characterization of LSST CCDs using realistic images, before first light", Proc. SPIE 10709, High Energy, Optical, and Infrared Detectors for Astronomy VIII, 107091L (12 July 2018); https://doi.org/10.1117/12.2314276
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Charge-coupled devices

Large Synoptic Survey Telescope

Point spread functions

Galactic astronomy

Stars

Silicon

Algorithm development

RELATED CONTENT

LSST optical beam simulator
Proceedings of SPIE (July 23 2014)
AIDA a software package for 2D model fitting analysis...
Proceedings of SPIE (September 24 2011)
Gaia in-orbit realignment: overview and data analysis
Proceedings of SPIE (September 21 2012)
Characterization of prototype LSST CCDs
Proceedings of SPIE (July 22 2008)

Back to Top