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Title: Astrometric calibration and performance of the Dark Energy Camera

Journal Article · · Publications of the Astronomical Society of the Pacific

We characterize the variation in photometric response of the Dark Energy Camera (DECam) across its 520~Mpix science array during 4 years of operation. These variations are measured using high signal-to-noise aperture photometry of $>10^7$ stellar images in thousands of exposures of a few selected fields, with the telescope dithered to move the sources around the array. A calibration procedure based on these results brings the RMS variation in aperture magnitudes of bright stars on cloudless nights down to 2--3 mmag, with <1 mmag of correlated photometric errors for stars separated by $$\ge20$$". On cloudless nights, any departures of the exposure zeropoints from a secant airmass law exceeding >1 mmag are plausibly attributable to spatial/temporal variations in aperture corrections. These variations can be inferred and corrected by measuring the fraction of stellar light in an annulus between 6" and 8" diameter. Key elements of this calibration include: correction of amplifier nonlinearities; distinguishing pixel-area variations and stray light from quantum-efficiency variations in the flat fields; field-dependent color corrections; and the use of an aperture-correction proxy. The DECam response pattern across the 2-degree field drifts over months by up to $$\pm7$$ mmag, in a nearly-wavelength-independent low-order pattern. We find no fundamental barriers to pushing global photometric calibrations toward mmag accuracy.

Research Organization:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); 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)
Contributing Organization:
DES Collaboration
Grant/Contract Number:
AC05-00OR22725; AC02-07CH11359; AC02-76SF00515; AST-1615555; SC0007901
OSTI ID:
1361381
Alternate ID(s):
OSTI ID: 1346375; OSTI ID: 1369280; OSTI ID: 1423239
Report Number(s):
arXiv:1703.01679; FERMILAB-PUB-17-057-AE; arXiv:1710.10943; FERMILAB-PUB-17-459-AE; KJ0402000; KJ0503000; ERKJ311; ERKJEPM
Journal Information:
Publications of the Astronomical Society of the Pacific, Vol. 129, Issue 977; ISSN 0004-6280
Publisher:
Astronomical Society of the PacificCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 39 works
Citation information provided by
Web of Science

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Cited By (13)

First Data Release of the All-sky NOAO Source Catalog journal August 2018
Astrometry and Occultation Predictions to Trans-Neptunian and Centaur Objects Observed within the Dark Energy Survey journal February 2019
First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release journal March 2019
LSST: From Science Drivers to Reference Design and Anticipated Data Products journal March 2019
The Dark Energy Survey: Data Release 1 journal November 2018
Dynamical Analysis of Three Distant Trans-Neptunian Objects with Similar Orbits journal November 2018
Overview of the DESI Legacy Imaging Surveys journal April 2019
The Dark Energy Survey: Data Release 1 text January 2018
LSST: from Science Drivers to Reference Design and Anticipated Data Products text January 2008
Overview of the DESI Legacy Imaging Surveys text January 2018
Dynamical Analysis of Three Distant Trans-Neptunian Objects with Similar Orbits text January 2018
First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release text January 2018
Astrometry and Occultation predictions to Trans-Neptunian and Centaur Objects observed within the Dark Energy Survey text January 2018

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