An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
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We present an algorithm to photometrically calibrate wide-field optical imaging surveys, which simultaneously solves for the calibration parameters and relative stellar fluxes using overlapping observations. The algorithm decouples the problem of "relative" calibrations from that of "absolute" calibrations; the absolute calibration is reduced to determining a few numbers for the entire survey. We pay special attention to the spatial structure of the calibration errors, allowing one to isolate particular error modes in downstream analyses. Applying this to the SDSS imaging data, we achieve ~1% relative calibration errors across 8500 deg 2 in griz ; the errors are ~2% for the u band. These errors are dominated by unmodeled atmospheric variations at Apache Point Observatory. These calibrations, dubbed "ubercalibration," are now public with SDSS Data Release 6 and will be a part of subsequent SDSS data releases.
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SDSS, PS1, and DES data taken in good photometric conditions have approached the LSST requirement of 1% photometric calibration.
“SDSS, PS1, and DES data taken in good photometric conditions have approached the LSST requirement of 1% photometric calibration ( Padmanabhan et al. 2008; Schla fl y et al. 2012; Burke et al. 2018 ) , although measurements with ground-based telescopes typically produce data with errors a factor of two or so larger.”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Padmanabhan et al. 2008
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FIRST-YEAR SLOAN DIGITAL SKY SURVEY-II SUPERNOVA RESULTS: HUBBLE DIAGRAM AND COSMOLOGICAL PARAMETERS
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THE PAN-STARRS 1 PHOTOMETRIC REFERENCE LADDER, RELEASE 12.01
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Self-citationRoss, A. J., Bautista, J., Tojeiro, R., Alam, S., Bailey, S., Burtin, E., Comparat, J., Dawson, K., de Mattia, A., Bourboux, H. D. M. D., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2416 · Cited by 182 · see citing works
Strong bimodality in the host halo mass of central galaxies from galaxy–galaxy lensing
Mandelbaum, R., Wang, W., Zu, Y., White, S. D. M., Henriques, B. M. B., & More, S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw188 · Cited by 180 · see citing works
Slosar, A., Font-Ribera, A., Pieri, M. M., Rich, J., Goff, J.-M. L., Aubourg, É., Brinkmann, J., Busca, N. G., Carithers, B., Charlassier, R., et al. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/09/001 · Cited by 179 · see citing works
Self-citation
- Authors
- Padmanabhan, N., Schlegel, D. J., Finkbeiner, D. P., Barentine, J. C., Blanton, M. R., Brewington, H. J., Gunn, J. E., Harvanek, M., Hogg, D. W., Ivezić, Ž., Johnston, D., Kent, S. M., Kleinman, S. J., Knapp, G. R., Krzesinski, J., Long, D., Neilsen, Jr., Nitta, A., Loomis, C., Lupton, R. H., Roweis, S., Snedden, S. A., Strauss, M. A., & Tucker, D. L.
- Affiliations
- Lawrence Berkeley National Laboratory (US)
- Princeton University (US)
- Udaipur Solar Observatory (IN)
- New York University (US)
- University of Washington (US)
- Jet Propulsion Laboratory (US)
- Fermi National Accelerator Laboratory (US)
- Subaru (Japan) (JP)
- University of Toronto (CA)
- ORCID
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2008-02-20
- Volume
- 674
- Issue
- 2
- Pages
- 1217-1233
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1572376656
- Cited by
- 591
- References
- 45
- Citations by year
- 2026: 8 · 2025: 9 · 2024: 14 · 2023: 24 · 2022: 19 · 2021: 21 · 2020: 12 · 2019: 33 · 2018: 38 · 2017: 40 · 2016: 60 · 2015: 50 · 2014: 52 · 2013: 42 · 2012: 60
- FWCI
- 52.64
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (acceptedVersion)
- University of North Texas Digital Library (University of North Texas) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- eScholarship (California Digital Library) (submittedVersion)
- Texas ScholarWorks (Texas Digital Library) (submittedVersion, other-oa)
- arXiv (Cornell University)
- Texas Digital Library (University of Texas)
- Lawrence Berkeley National Laboratory
- Funders
- National Science Foundation
- U.S. Department of Energy
- National Aeronautics and Space Administration
- Alfred P. Sloan Foundation
- Princeton University
- Ohio State University
- University of Washington
- Johns Hopkins University
- University of Pittsburgh
- Case Western Reserve University
- Drexel University
- Universität Basel
- University of Portsmouth
- New Mexico State University
- University of Cambridge
- Chinese Academy of Sciences
- Max-Planck-Gesellschaft
- Max-Planck-Institut für Astronomie
- U.S. Naval Observatory
- Fermilab
- Los Alamos National Laboratory
- Topics
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Engineering › Computational Mechanics › Astronomical Observations and Instrumentation
- Keywords
- photometric calibration, Sloan Digital Sky Survey, wide-field optical imaging, relative calibration, absolute calibration, overlapping observations, calibration error, atmospheric variability, Apache Point Observatory
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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