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Cited by 318

The DOI matches its Crossref record; 49 of the 49 references it cites were found in a registry or an index.

Sloan Digital Sky Survey Standard Star Catalog for Stripe 82: The Dawn of Industrial 1% Optical Photometry

Open access
Ivezić, Željko, Smith, J. Allyn, Miknaitis, Gajus, Lin, Huan, Tucker, Douglas, Lupton, Robert H., Gunn, James E., Knapp, Gillian R., Strauss, Michael A., Sesar, Branimir, Doi, Mamoru, Tanaka, Masayuki, Fukugita, Masataka, Holtzman, Jon, Kent, Steve, Yanny, Brian, Schlegel, David, Finkbeiner, Douglas, Padmanabhan, Nikhil, Rockosi, Constance M., Jurić, Mario, Bond, Nicholas, Lee, Brian, Stoughton, Chris, Jester, Sebastian, Harris, Hugh, Harding, Paul, Morrison, Heather, Brinkmann, Jon, Schneider, Donald P., York, Donald·2007·The Astronomical Journal

Abstract

We describe a standard star catalog constructed using multiple SDSS photometric observations (at least four per band, with a median of 10) in the ugriz system. The catalog includes 1.01 million nonvariable unresolved objects from the equatorial stripe 82 (|δ J2000.0 | < 1.266°) in the right ascension range 20 h 34 m -4 h 00 m and with the corresponding r -band (approximately Johnson V -band) magnitudes in the range 14-22. The distributions of measurements for individual sources demonstrate that the photometric pipeline correctly estimates random photometric errors, which are below 0.01 mag for stars brighter than 19.5, 20.5, 20.5, 20, and 18.5 in ugriz , respectively (about twice as good as for individual SDSS runs). Several independent tests of the internal consistency suggest that the spatial variation of photometric zero points is not larger than ∼0.01 mag (rms). In addition to being the largest available data set with optical photometry internally consistent at the ∼1% level, this catalog provides a practical definition of the SDSS photometric system. Using this catalog, we show that photometric zero points for SDSS observing runs can be calibrated within a nominal uncertainty of 2% even for data obtained through 1 mag thick clouds, and we demonstrate the existence of He and H white dwarf sequences using photometric data alone. Based on the properties of this catalog, we conclude that upcoming large-scale optical surveys such as the Large Synoptic Survey Telescope will be capable of delivering robust 1% photometry for billions of sources.

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Metadata

Authors
Ivezić, Ž., Smith, J. A., Miknaitis, G., Lin, H., Tucker, D., Lupton, R. H., Gunn, J. E., Knapp, G. R., Strauss, M. A., Sesar, B., Doi, M., Tanaka, M., Fukugita, M., Holtzman, J., Kent, S., Yanny, B., Schlegel, D., Finkbeiner, D., Padmanabhan, N., Rockosi, C. M., Jurić, M., Bond, N., Lee, B., Stoughton, C., Jester, S., Harris, H., Harding, P., Morrison, H., Brinkmann, J., Schneider, D. P., & York, D.
Venue
The Astronomical Journal
Published
2007-07-10
Volume
134
Issue
3
Pages
973-998
ISSN
  • 0004-6256 (ISSN-L)
  • 1538-3881
OpenAlex
W1624842220
Cited by
318
References
49
FWCI
12.48
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Sloan Digital Sky Survey Standard Star Catalog for Stripe 82: The Dawn of Industrial 1% Optical Photometry. https://app.cochat.ai/papers/10.1086/519976
The paper
Ivezić, Ž., Smith, J. A., Miknaitis, G., Lin, H., Tucker, D., Lupton, R. H., Gunn, J. E., Knapp, G. R., Strauss, M. A., Sesar, B., Doi, M., Tanaka, M., Fukugita, M., Holtzman, J., Kent, S., Yanny, B., Schlegel, D., Finkbeiner, D., Padmanabhan, N., . . . York, D. (2007). Sloan Digital Sky Survey Standard Star Catalog for Stripe 82: The Dawn of Industrial 1% Optical Photometry. The Astronomical Journal. https://doi.org/10.1086/519976

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.