A survey of z>5.7 quasars in the Sloan Digital Sky Survey.: III.: Discovery of five additional quasars

被引:328
作者
Fan, XH
Hennawi, JF
Richards, GT
Strauss, MA
Schneider, DP
Donley, JL
Young, JE
Annis, J
Lin, H
Lampeitl, H
Lupton, RH
Gunn, JE
Knapp, GR
Brandt, WN
Anderson, S
Bahcall, NA
Brinkmann, J
Brunner, RJ
Fukugita, M
Szalay, AS
Szokoly, GP
York, DG
机构
[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[2] Princeton Univ Observ, Princeton, NJ 08544 USA
[3] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[5] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[6] Apache Point Observ, Sunspot, NM 88349 USA
[7] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
[8] Univ Illinois, Natl Ctr Supercomp Applicat, Urbana, IL 61801 USA
[9] Univ Tokyo, Inst Cosm Ray Res, Midori Ku, Tokyo 1888502, Japan
[10] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[11] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[12] Univ Chicago, Ctr Astron & Astrophys, Chicago, IL 60637 USA
关键词
quasars : absorption lines; quasars : emission lines; quasars : general;
D O I
10.1086/422434
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the discovery of five new quasars at z > 5.7, selected from the multicolor imaging data of the Sloan Digital Sky Survey (SDSS). Three of them, at redshifts 5.93, 6.07, and 6.22, were selected from similar to1700 deg(2) of new SDSS Main Survey imaging in the northern Galactic cap. An additional quasar, at redshift 5.85, was discovered by co-adding the data obtained in the Fall Equatorial Stripe in the SDSS Southern Survey Region. The fifth object, at redshift 5.80, is selected from a nonstandard SDSS scan in the southern Galactic cap outside the Main Survey area. The spectrum of SDSS J162331.81+ 311200.5 ( z = 6.22) shows a complete Gunn-Peterson trough at z(abs) > 5.95, similar to the troughs detected in the other three z greater than or similar to 6.2 quasars known. We present a composite spectrum of the z > 5.7 quasars discovered in the SDSS to date. The average emission-line and continuum properties of z similar to 6 quasars exhibit no significant evolution compared with those at low redshift. Using a complete sample of nine z > 5.7 quasars, we find that the density of quasars with M-1450 < -26.7 at z similar to 6 is (6 +/- 2) x 10(-10) Mpc(-3) (H-0 = 65 km s(-1) Mpc(-1), Omega = 0.35, and Lambda = 0.65), consistent with our previous estimates. The luminosity distribution of the sample is fitted with a power-law luminosity function Psi( L) proportional to L-3.2 +/- 0.7, somewhat steeper than but consistent with our previous estimates.
引用
收藏
页码:515 / 522
页数:8
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