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A fringe projector-based study of the Brighter-Fatter Effect in LSST CCDs
In order to achieve the goals of the Large Synoptic Survey Telescope for Dark Energy science requires a detailed understanding of CCD sensor effects. One such sensor effect is the Point Spread Function (PSF) increasing with flux, alternatively called the `Brighter-Fatter Effect.' Here a novel approach was tested to perform the PSF measurements in the context of the Brighter-Fatter Effect employing a Michelson interferometer to project a sinusoidal fringe pattern onto the CCD. The Brighter-Fatter effect predicts that the fringe pattern should become asymmetric in the intensity pattern as the brighter peaks corresponding to a larger flux are smeared by a larger PSF. By fitting the data with a model that allows for a changing PSF, the strength of the Brighter-Fatter effect can be evaluated.
- Univ. of Arkansas, Fayetteville, AR (United States). Dept. of Physics; Brookhaven National Lab. (BNL), Upton, NY (United States). Physics Dept.
- Brookhaven National Lab. (BNL), Upton, NY (United States). Physics Dept.
- Publication Date:
- Report Number(s):
Journal ID: ISSN 1748-0221
- Grant/Contract Number:
- Accepted Manuscript
- Journal Name:
- Journal of Instrumentation
- Additional Journal Information:
- Journal Volume: 12; Journal Issue: 09; Conference: Precision Astronomy with Fully Depleted CCDs, Upton, NY (United States), 01-02 Dec 2016; Journal ID: ISSN 1748-0221
- Institute of Physics (IOP)
- Research Org:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Org:
- USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- Country of Publication:
- United States
- 79 ASTRONOMY AND ASTROPHYSICS
- OSTI Identifier: