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SDSS data management and photometric quality assessment
Open accessAbstract
We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color‐color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg 2 patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ∼0.01 mag in the g,r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root‐mean‐scatter for zeropoint offsets). (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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Citations
Cites
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Self-citationSpectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
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Self-citationPhotometric Separation of Stellar Properties Using SDSS Filters
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Self-citationSignatures of galaxy mergers in the Milky Way: Here, there and everywhere
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Cited by
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341
Self-citationEisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · The Astrophysical Journal · doi:10.1086/466512 · Cited by 4,629
Self-citationThe 2.5 m Telescope of the Sloan Digital Sky Survey
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Self-citationBaryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample
Percival, W. J., Reid, B. A., Eisenstein, D. J., Bahcall, N. A., Budavari, T., Frieman, J. A., Fukugita, M., Gunn, J. E., Ivezić, Ž., Knapp, G. R., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15812.x · Cited by 1,846
“The images were reduced (Lupton et al. 2001; Stoughton et al. 2002; Pier et al. 2003; Ivezic et al. 2004) and calibrated (Lupton, Gunn & Szalay 1999; Hogg et al. 2001; Smith et al. 2002; Tucker et al. 2006), and galaxies were selected in two ways for follow-up spectroscopy.”
MethodSelf-citationA CATALOG OF QUASAR PROPERTIES FROM SLOAN DIGITAL SKY SURVEY DATA RELEASE 7
Shen, Y., Richards, G. T., Strauss, M. A., Hall, P. B., Schneider, D. P., Snedden, S., Bizyaev, D., Brewington, H., Malanushenko, V., Malanushenko, E., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/194/2/45 · Cited by 1,517
Self-citation
Metadata
- Authors
- Ivezić, Ž., Lupton, R. H., Schlegel, D., Boroski, B., Adelman‐McCarthy, J., Yanny, B., Kent, S., Stoughton, C., Finkbeiner, D., Padmanabhan, N., Rockosi, C. M., Gunn, J. E., Knapp, G. R., Strauss, M. A., Richards, G. T., Eisenstein, D., Nicinski, T., Kleinman, S. J., Krzesinski, J., Newman, P. R., Snedden, S., Thakar, A. R., Szalay, A., Munn, J. A., Smith, J. A., Tucker, D., & Lee, B. C.
- Venue
- Astronomische Nachrichten
- Publisher
- Wiley
- Published
- 2004-10
- Volume
- 325
- Issue
- 6-8
- Pages
- 583-589
- ISSN
- 0004-6337 (ISSN-L)
- 1521-3994
- OpenAlex
- W2104713387
- Cited by
- 469
- References
- 22
- FWCI
- 57.52
- Type
- journal article
- Language
- en
- Open access
- green
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