The 2.5 m Telescope of the Sloan Digital Sky Survey
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We describe the design, construction, and performance of the Sloan Digital Sky Survey telescope located at Apache Point Observatory. The telescope is a modified two-corrector Ritchey-Chrétien design with a 2.5 m, f/2.25 primary, a 1.08 m secondary, a Gascoigne astigmatism corrector, and one of a pair of interchangeable highly aspheric correctors near the focal plane, one for imaging and the other for spectroscopy. The final focal ratio is f/5. The telescope is instrumented by a wide-area, multiband CCD camera and a pair of fiber-fed double spectrographs. Novel features of the telescope include the following: (1) A 3° diameter (0.65 m) focal plane that has excellent image quality and small geometric distortions over a wide wavelength range (3000-10,600 Å) in the imaging mode, and good image quality combined with very small lateral and longitudinal color errors in the spectroscopic mode. The unusual requirement of very low distortion is set by the demands of time-delay-and-integrate (TDI) imaging. (2) Very high precision motion to support open-loop TDI observations. (3) A unique wind baffle/enclosure construction to maximize image quality and minimize construction costs. The telescope had first light in 1998 May and began regular survey operations in 2000.
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SDSS has an effective étendue of only 5.9 m2 deg2.
“For example, the SDSS, with its 2.5 m telescope ( Gunn et al. 2006 ) and a camera with 30 imaging CCDs ( Gunn et al. 1998 ) , has an effective étendue of only 5.9 m 2 deg 2 .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Gunn et al. 2006
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Self-citationExploring the Variable Sky with the Sloan Digital Sky Survey
Sesar, B., Ivezić, Ž., Lupton, R. H., Jurić, M., Gunn, J. E., Knapp, G. R., De Lee, N., Smith, J. A., Miknaitis, G., Lin, H., et al. (2007) · The Astronomical Journal · doi:10.1086/521819 · Cited by 360 · see citing works
Self-citationA systematic search for changing-look quasars in SDSS
MacLeod, C. L., Ross, N. P., Lawrence, A., Goad, M., Horne, K., Burgett, W., Chambers, K. C., Flewelling, H., Hodapp, K., Kaiser, N., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2997 · Cited by 323 · see citing works
Mackereth, J. T., Schiavon, R. P., Pfeffer, J., Hayes, C. R., Bovy, J., Anguiano, B., Prieto, C. A., Hasselquist, S., Holtzman, J., Johnson, J. A., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2955 · Cited by 285 · see citing works
Grier, C. J., Trump, J. R., Shen, Y., Horne, K., Kinemuchi, K., McGreer, I. D., Starkey, D. A., Brandt, W. N., Hall, P. B., Kochanek, C. S., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa98dc · Cited by 244 · see citing works
Self-citationTHE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: TECHNICAL OVERVIEW
Shen, Y., Brandt, W. N., Dawson, K. S., Hall, P. B., McGreer, I. D., Anderson, S. F., Chen, Y., Denney, K. D., Eftekharzadeh, S., Fan, X., et al. (2014) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/216/1/4 · Cited by 210 · see citing works
Self-citationLeistedt, B., Peiris, H. V., & Roth, N. (2014) · Physical Review Letters · doi:10.1103/physrevlett.113.221301 · Cited by 119 · see citing works
Self-supervised Representation Learning for Astronomical Images
Hayat, M. A., Stein, G., Harrington, P., Lukić, Z., & Mustafa, M. (2021) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/abf2c7 · Cited by 79 · see citing works
Fernández-Alvar, E., Carigi, L., Schuster, W. J., Hayes, C. R., Ávila-Vergara, N., Majewski, S. R., Allende Prieto, C., Beers, T. C., Sánchez, S. F., Zamora, O., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aa9ced · Cited by 68 · see citing works
THE VARIABLE SKY OF DEEP SYNOPTIC SURVEYS
Ridgway, S. T., Matheson, T., Mighell, K. J., Olsen, K. A., & Howell, S. B. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/796/1/53 · Cited by 33 · see citing works
- Authors
- Gunn, J. E., Siegmund, W. A., Mannery, E. J., Owen, R. E., Hull, C. L., Leger, R. F., Carey, L. N., Knapp, G. R., York, D. G., Boroski, W. N., Kent, S. M., Lupton, R. H., Rockosi, C. M., Evans, M. L., Waddell, P., Anderson, J. E., Annis, J., Barentine, J. C., Bartoszek, L. M., Bastian, S., Bracker, S. B., Brewington, H. J., Briegel, C. I., Brinkmann, J., Brown, Y. J., Carr, M. A., Czarapata, P. C., Drennan, C. C., Dombeck, T., Federwitz, G. R., Gillespie, B. A., Gonzales, C., Hansen, S. U., Harvanek, M., Hayes, J., Jordan, W., Kinney, E., Klaene, M., Kleinman, S. J., Kron, R. G., Kresinski, J., Lee, G., Limmongkol, S., Lindenmeyer, C. W., Long, D. C., Loomis, C. L., McGehee, P. M., Mantsch, P. M., Neilsen, Jr., Neswold, R. M., Newman, P. R., Nitta, A., Peoples, Jr., Pier, J. R., Prieto, P. S., Prosapio, A., Rivetta, C., Schneider, D. P., Snedden, S., & Wang, S.-I.
- Affiliations
- Princeton University (US)
- University of Washington (US)
- Fermi National Accelerator Laboratory (US)
- University of Chicago (US)
- University of California, Santa Cruz (US)
- Los Alamos National Laboratory (US)
- United States Naval Observatory (US)
- Pennsylvania State University (US)
- ORCID
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2006-04
- Volume
- 131
- Issue
- 4
- Pages
- 2332-2359
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2063568047
- Cited by
- 2,373
- References
- 57
- Citations by year
- 2026: 79 · 2025: 143 · 2024: 140 · 2023: 137 · 2022: 177 · 2021: 148 · 2020: 158 · 2019: 155 · 2018: 140 · 2017: 125 · 2016: 181 · 2015: 119 · 2014: 92 · 2013: 87 · 2012: 98
- FWCI
- 110.71
- Type
- journal article
- Language
- en
- Open access
- hybrid
- doi.org
- Licence
- public-domain
- Locations
- The Astronomical Journal (publishedVersion, public-domain)
- arXiv (Cornell University) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation
- U.S. Department of Energy
- National Aeronautics and Space Administration
- Alfred P. Sloan Foundation
- Princeton University
- University of Washington
- Johns Hopkins University
- University of Pittsburgh
- University of Portsmouth
- New Mexico State University
- 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 › Atomic and Molecular Physics, and Optics › Adaptive optics and wavefront sensing
- Physical Sciences › Engineering › Biomedical Engineering › Advanced optical system design
- Keywords
- Apache Point Observatory, Ritchey-Chretien telescope, fiber-fed spectrograph, image quality, color error
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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