Photometric cross-calibration of the SDSS Stripe 82 Standard Stars catalogue with Gaia EDR3, and comparison with Pan-STARRS1, DES, CFIS, and GALEX catalogues

Author:

Thanjavur Karun1ORCID,Ivezić Željko2ORCID,Allam Sahar S3ORCID,Tucker Douglas L3ORCID,Smith J Allyn4ORCID,Gwyn Stephen5

Affiliation:

1. Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road, Victoria, BC V8P 5C2, Canada

2. Department of Astronomy and the DiRAC Institute, University of Washington, 3910 15th Avenue NE, Seattle, WA 98195, USA

3. Fermi National Accelerator Laboratory, Batavia, IL 60510, USA

4. Department of Physics, Engineering and Astronomy, Austin Peay State University, 601 College St., Clarksville, TN 37044, USA

5. National Research Council, Canadian Astronomy Data Centre, Victoria, BC V9E 2E7, Canada

Abstract

ABSTRACT We extend the SDSS Stripe 82 Standard Stars catalogue with post-2007 SDSS imaging data. This improved version lists averaged SDSS ugriz photometry for nearly a million stars brighter than r ∼ 22 mag. With 2–3 times more measurements per star, random errors are 1.4–1.7 times smaller than in the original catalogue, and about three times smaller than for individual SDSS runs. Random errors in the new catalogue are $\lesssim$0.01 mag for stars brighter than 20.0, 21.0, 21.0, 20.5, and 19.0 mag in u, g, r, i, and z-bands, respectively. We achieve this error threshold by using the Gaia Early Data Release 3 (EDR3) Gmag photometry to derive grey photometric zeropoint corrections, as functions of RA and Declination, for the SDSS catalogue, and use the Gaia BP–RP colour to derive corrections in the ugiz bands, relative to the r-band. The quality of the recalibrated photometry, tested against Pan-STARRS1, DES, CFIS, and GALEX surveys, indicates spatial variations of photometric zeropoints ≦ 0.01 mag (rms), with typical values of 3–7 millimag in the RA, and 1–2 millimag in the Declination directions, except for $\lesssim$6 millimag scatter in the u-band. We also report a few minor photometric problems with other surveys considered here, including a magnitude-dependent ∼0.01 mag bias between 16 ≤ GGaia ≤ 20 in the Gaia EDR3. Our new, publicly available catalogue offers robust calibration of ugriz photometry below 1 per cent level, and will be helpful during the commissioning of the Vera C. Rubin Observatory Legacy Survey of Space and Time.

Funder

University of Washington College of Arts and Sciences

Washington Research Foundation

U.S. Department of Energy

Office of Science

University of Utah

Carnegie Mellon University

Johns Hopkins University

University of Tokyo

Lawrence Berkeley National Laboratory

New Mexico State University

New York University

University of Notre Dame

Pennsylvania State University

University of Arizona

University of Colorado Boulder

University of Portsmouth

University of Virginia

University of Washington

Vanderbilt University

Yale University

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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