The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
The Sloan Digital Sky Survey Quasar Survey: Quasar Luminosity Function from Data Release 3
Open accessAbstract
We determine the number counts and z = 0-5 luminosity function for a well-defined, homogeneous sample of quasars from the Sloan Digital Sky Survey (SDSS). We conservatively define the most uniform statistical sample possible, consisting of 15,343 quasars within an effective area of 1622 deg 2 that was derived from a parent sample of 46,420 spectroscopically confirmed broad-line quasars in the 5282 deg 2 of imaging data from SDSS Data Release 3. The sample extends from i = 15 to 19.1 at z ≲ 3 and to i = 20.2 for z ≳ 3. The number counts and luminosity function agree well with the results of the Two Degree Field QSO Redshift Survey (2QZ) at redshifts and luminosities at which the SDSS and 2QZ quasar samples overlap, but the SDSS data probe to much higher redshifts than does the 2QZ sample. The number density of luminous quasars peaks between redshifts 2 and 3, although uncertainties in the selection function in this range do not allow us to determine the peak redshift more precisely. Our best-fit model has a flatter bright-end slope at high redshift than at low redshift. For z < 2.4 the data are best fit by a redshift-independent slope of β = -3.1 [Φ( L ) ∝ L β ]. Above z = 2.4 the slope flattens with redshift to β ≳ -2.37 at z = 5. This slope change, which is significant at the ≳5 σ level, must be accounted for in models of the evolution of accretion onto supermassive black holes.
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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-citationSpergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
The 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 2×
“Vega-based photometric systems require an additional correction term: B − g is ∼ 0.14 (Fukugita et al. 1996).”
BackgroundInfluentialSelf-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
Self-citationAstrometric Calibration of the Sloan Digital Sky Survey
Pier, J. R., Munn, J. A., Hindsley, R. B., Hennessy, G. S., Kent, S. M., Lupton, R. H., & Ivezić, Ž. (2003) · The Astronomical Journal · doi:10.1086/346138 · Cited by 908
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THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III
Dawson, K. S., Schlegel, D. J., Ahn, C. P., Anderson, S. F., Aubourg, É., Bailey, S., Barkhouser, R. H., Bautista, J. E., Beifiori, A., Berlind, A. A., et al. (2013) · The Astronomical Journal · doi:10.1088/0004-6256/145/1/10 · Cited by 2,051
Self-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-citationSEGUE: A SPECTROSCOPIC SURVEY OF 240,000 STARS WITH g = 14-20
Yanny, B., Rockosi, C., Newberg, H. J., Knapp, G. R., Adelman-McCarthy, J. K., Alcorn, B., Allam, S., Prieto, C. A., An, D., Anderson, K. S. J., et al. (2009) · The Astronomical Journal · doi:10.1088/0004-6256/137/5/4377 · Cited by 1,162
“…science program consists of constructing a large three-dimensional map of the universe and constraining cosmological models; see, e.g. Becker et al. (2001); Blanton et al. (2003b); Fan et al. (2003); Tremonti et al. (2004); Tegmark et al. (2004); Eisenstein et al. (2005); Richards et al. (2006).”
BackgroundSelf-citationA NEW CALCULATION OF THE IONIZING BACKGROUND SPECTRUM AND THE EFFECTS OF He II REIONIZATION
Faucher-Giguère, C.-A., Lidz, A., Zaldarriaga, M., & Hernquist, L. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/703/2/1416 · Cited by 699
Active galactic nuclei: what’s in a name?
Padovani, P., Alexander, D. M., Assef, R. J., De Marco, B., Giommi, P., Hickox, R. C., Richards, G. T., Smolčić, V., Hatziminaoglou, E., Mainieri, V., et al. (2017) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-017-0102-9 · Cited by 666
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Metadata
- Authors
- Richards, G. T., Strauss, M. A., Fan, X., Hall, P. B., Jester, S., Schneider, D. P., Vanden Berk, D. E., Stoughton, C., Anderson, S. F., Brunner, R. J., Gray, J., Gunn, J. E., Ivezić, Ž., Kirkland, M. K., Knapp, G. R., Loveday, J., Meiksin, A., Pope, A., Szalay, A. S., Thakar, A. R., Yanny, B., York, D. G., Barentine, J. C., Brewington, H. J., Brinkmann, J., Fukugita, M., Harvanek, M., Kent, S. M., Kleinman, S. J., Krzesiński, J., Long, D. C., Lupton, R. H., Nash, T., Neilsen, Jr., Nitta, A., Schlegel, D. J., & Snedden, S. A.
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2006-06
- Volume
- 131
- Issue
- 6
- Pages
- 2766-2787
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2062713883
- Cited by
- 876
- References
- 5
- FWCI
- 32.78
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Richards, G. T., Strauss, M. A., Fan, X., Hall, P. B., Jester, S., Schneider, D. P., Vanden Berk, D. E., Stoughton, C., Anderson, S. F., Brunner, R. J., Gray, J., Gunn, J. E., Ivezić, Ž., Kirkland, M. K., Knapp, G. R., Loveday, J., Meiksin, A., Pope, A., Szalay, A. S., . . . Snedden, S. A. (2006). The Sloan Digital Sky Survey Quasar Survey: Quasar Luminosity Function from Data Release 3. The Astronomical Journal. https://doi.org/10.1086/503559
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