The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
Open accessAbstract
We describe the algorithm for selecting quasar candidates for optical spectroscopy in the Sloan Digital Sky Survey. Quasar candidates are selected via their non-stellar colors in "ugriz" broad-band photometry, and by matching unresolved sources to the FIRST radio catalogs. The automated algorithm is sensitive to quasars at all redshifts lower than z=5.8. Extended sources are also targeted as low-redshift quasar candidates in order to investigate the evolution of Active Galactic Nuclei (AGN) at the faint end of the luminosity function. Nearly 95% of previously known quasars are recovered (based on 1540 quasars in 446 square degrees). The overall completeness, estimated from simulated quasars, is expected to be over 90%, whereas the overall efficiency (quasars:quasar candidates) is better than 65%. The selection algorithm targets ultraviolet excess quasars to i^*=19.1 and higher-redshift (z>3) quasars to i^*=20.2, yielding approximately 18 candidates per square degree. In addition to selecting ``normal'' quasars, the design of the algorithm makes it sensitive to atypical AGN such as Broad Absorption Line quasars and heavily reddened quasars.
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Cites
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
Self-citationThe Sloan Digital Sky Survey Photometric System
Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P. (1996) · The Astronomical Journal · doi:10.1086/117915 · Cited by 3,033 · cited 3×
“The imaging survey is done in five broad bands, ugriz (Fukugita et al. 1996; Stoughton et al. 2002), that were specially designed for the survey.”
BackgroundMethodSelf-citationThe Sloan Digital Sky Survey Photometric Camera
Gunn, J. E., Carr, M., Rockosi, C., Sekiguchi, M., Berry, K., Elms, B., de Haas, E., Ivezić, Ž., Knapp, G., Lupton, R., et al. (1998) · The Astronomical Journal · doi:10.1086/300645 · Cited by 1,692
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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-citationLSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357
“…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 al. 2012).”
BackgroundSelf-citationThe 2.5 m Telescope of the Sloan Digital Sky Survey
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., et al. (2006) · The Astronomical Journal · doi:10.1086/500975 · Cited by 2,373
Self-citationSpectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
Strauss, M. A., Weinberg, D. H., Lupton, R. H., Narayanan, V. K., Annis, J., Bernardi, M., Blanton, M., Burles, S., Connolly, A. J., Dalcanton, J., et al. (2002) · The Astronomical Journal · doi:10.1086/342343 · Cited by 1,909
Self-citationK -Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared
Blanton, M. R., & Roweis, S. (2007) · The Astronomical Journal · doi:10.1086/510127 · Cited by 1,579
Metadata
- Authors
- Richards, G. T., Fan, X., Newberg, H. J., Strauss, M. A., Vanden Berk, D. E., Schneider, D. P., Yanny, B., Boucher, A., Burles, S., Frieman, J. A., Gunn, J. E., Hall, P. B., Ivezić, Ž., Kent, S., Loveday, J., Lupton, R. H., Rockosi, C. M., Schlegel, D. J., Stoughton, C., SubbaRao, M., & York, D. G.
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2002-06
- Volume
- 123
- Issue
- 6
- Pages
- 2945-2975
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2037502800
- Cited by
- 1,003
- References
- 3
- FWCI
- 34.91
- Type
- journal article
- Language
- en
- Open access
- green
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- Richards, G. T., Fan, X., Newberg, H. J., Strauss, M. A., Vanden Berk, D. E., Schneider, D. P., Yanny, B., Boucher, A., Burles, S., Frieman, J. A., Gunn, J. E., Hall, P. B., Ivezić, Ž., Kent, S., Loveday, J., Lupton, R. H., Rockosi, C. M., Schlegel, D. J., Stoughton, C., . . . York, D. G. (2002). Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample. The Astronomical Journal. https://doi.org/10.1086/340187
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