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The Sloan Digital Sky Survey Photometric System
Abstract
This paper describes the Sloan Digital Sky Survey photometric system, a new five-color (u‧ g‧ r‧ i‧ z‧) wide-band CCD system with wavelength coverage from 3000 to 11 000 Å. The zero points will be based on an updated version of the spectrophotometric ABv system. This updated calibration, designated as AB95, is presented in this paper.
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“The LSST fi lter complement ( ugrizy ; see Figure 4 ) is modeled after the SDSS system ( Fukugita et al. 1996 ) because of its demonstrated success in a wide variety of applications, including photometric redshifts of galaxies ( Budavári et al. 2003 ) , separation of stellar populations ( Lenz et al. 1998; Helmi et al. 2003 ) , and photometric selection of quasars ( Richards et al. 2002; Ross et”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Fukugita et al. 1996
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Self-citationWINGS: a WIde-field Nearby Galaxy-cluster Survey
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Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology
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“The SDSS I/II/III used a dedicated 2.5 m wide-field telescope (Gunn et al. 2006) with a drift-scan camera with 30 2048×2048 CCDs (Gunn et al. 1998) to image the sky in five broad bands (ugriz; Fukugita et al. 1996).”
MethodInfluentialSelf-citationThe build-up of the colour-magnitude relation as a function of environment
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Self-citationObserving the Dark Matter Density Profile of Isolated Galaxies
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Galaxy And Mass Assembly (GAMA): The input catalogue and star–galaxy separation
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Metadata
- Authors
- Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P.
- Affiliations
- Kyoto University (JP)
- The University of Tokyo (JP)
- Princeton University (US)
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 1996-04
- Volume
- 111
- Pages
- 1748
- ISSN
- 0004-6256 (ISSN-L)
- OpenAlex
- W1979742375
- Cited by
- 3,033
- References
- 0
- Citations by year
- 2026: 57 · 2025: 72 · 2024: 68 · 2023: 87 · 2022: 87 · 2021: 66 · 2020: 70 · 2019: 94 · 2018: 125 · 2017: 121 · 2016: 150 · 2015: 108 · 2014: 138 · 2013: 140 · 2012: 161
- FWCI
- 40.05
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- The Astronomical Journal (publishedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- 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 › Physics and Astronomy › Astronomy and Astrophysics › Astronomical Observations and Instrumentation
- Keywords
- Sloan Digital Sky Survey, photometric systems, photometric zero points, spectrophotometric calibration
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.
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