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Title: Instrumental response model and detrending for the Dark Energy Camera

Journal Article · · Publ.Astron.Soc.Pac.

We describe the model for the mapping from sky brightness to the digital output of the Dark Energy Camera, and the algorithms adopted by the Dark Energy Survey (DES) for inverting this model to obtain photometric measures of celestial objects from the raw camera output. The calibration aims for fluxes that are uniform across the camera field of view and across the full angular and temporal span of the DES observations, approaching the accuracy limits set by shot noise for the full dynamic range of DES observations. The DES pipeline incorporates several substantive advances over standard detrending techniques, including: principal-components-based sky and fringe subtraction; correction of the "brighter-fatter" nonlinearity; use of internal consistency in on-sky observations to disentangle the influences of quantum efficiency, pixel-size variations, and scattered light in the dome flats; and pixel-by-pixel characterization of instrument spectral response, through combination of internal-consistency constraints with auxiliary calibration data. This article provides conceptual derivations of the detrending/calibration steps, and the procedures for obtaining the necessary calibration data. Other publications will describe the implementation of these concepts for the DES operational pipeline, the detailed methods, and the validation that the techniques can bring DECam photometry and astrometry within ~2 mmag and ~3 mas, respectively, of fundamental atmospheric and statistical limits. The DES techniques should be broadly applicable to wide-field imagers.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1469017
Report Number(s):
arXiv:1706.09928; FERMILAB-PUB-17-208-AE; 1608214
Journal Information:
Publ.Astron.Soc.Pac., Vol. 129
Country of Publication:
United States
Language:
English

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Cited By (11)

The Large Synoptic Survey Telescope and Milky Way Science journal July 2017
First Data Release of the All-sky NOAO Source Catalog journal August 2018
First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release journal March 2019
Dark Energy Survey Year 1 Results: Detection of Intracluster Light at Redshift ∼ 0.25 journal April 2019
The Dark Energy Survey: Data Release 1 journal November 2018
A Search for Optical Emission from Binary Black Hole Merger GW170814 with the Dark Energy Camera journal March 2019
GROWTH on S190426c: Real-time Search for a Counterpart to the Probable Neutron Star–Black Hole Merger using an Automated Difference Imaging Pipeline for DECam journal August 2019
The Dark Energy Survey: Data Release 1 text January 2018
The Large Synoptic Survey Telescope and Milky Way Science text January 2017
First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release text January 2018
Dark Energy Survey Year 1 results: Detection of Intra-cluster Light at Redshift $\sim$ 0.25 text January 2018

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