High-redshift quasars found in Sloan Digital Sky Survey commissioning data. II. The spring Equatorial Stripe

被引:66
作者
Fan, XH
Strauss, MA
Schneider, DP
Gunn, JE
Lupton, RH
Anderson, SF
Voges, W
Margon, B
Annis, J
Bahcall, NA
Brinkmann, J
Brunner, RJ
Carr, MA
Csabai, I
Doi, M
Frieman, JA
Fukugita, M
Hennessy, GS
Hindsley, RB
Ivezic, Z
Knapp, GR
Lamb, DQ
McKay, TA
Munn, JA
Newberg, HJ
Pauls, AG
Pier, JR
Rechenmacher, R
Richards, GT
Rockosi, CM
Stoughton, C
Szalay, AS
Thakar, AR
Tucker, DL
Waddell, P
York, DG
机构
[1] Princeton Univ Observ, Princeton, NJ 08544 USA
[2] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[3] Max Planck Inst Extraterr Phys, D-85750 Garching, Germany
[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[5] Apache Point Observ, Sunspot, NM 88349 USA
[6] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[7] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[8] Eotvos Lorand Univ, Dept Phys Complex Syst, H-1117 Budapest, Hungary
[9] Univ Tokyo, Sch Sci, Dept Astron, Tokyo 1130033, Japan
[10] Univ Chicago, Ctr Astron & Astrophys, Chicago, IL 60637 USA
[11] Univ Tokyo, Inst Cosm Ray Res, Tanashi, Tokyo 1888502, Japan
[12] Inst Adv Study, Princeton, NJ 08540 USA
[13] USN Observ, Washington, DC 20392 USA
[14] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[15] USN Observ, Flagstaff Stn, Flagstaff, AZ 86002 USA
[16] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[17] Univ Tokyo, Sch Sci, Res Ctr Early Universe, Tokyo 1130033, Japan
关键词
quasars : general; surveys;
D O I
10.1086/301191
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This is the second paper in a series aimed at finding high-redshift quasars from five-color (u'g'r'i'z') imaging data taken along the Celestial Equator by the Sloan Digital Sky Survey (SDSS) during its commissioning phase. In this paper, we present 22 high-redshift quasars (z > 3.6) discovered from similar to 250 deg(2) of data in the spring Equatorial Stripe, plus photometry for two previously known high-redshift quasars in the same region of the sky. Our success rate in identifying high-redshift quasars is 68%. Five of the newly discovered quasars have redshifts higher than 4.6 (z = 4.62, 4.69, 4.70, 4.92, and 5.03). All the quasars have i* < 20.2 with absolute magnitude -28.8 < M < M(B) -26.1 (h = 0.5, q(0) = 0.5). Several of the quasars show unusual emission and absorption features in their spectra, including an object at z = 4.62 without detectable emission lines, and a broad absorption line (BAL) quasar at z = 4.92.
引用
收藏
页码:1 / 11
页数:11
相关论文
共 29 条
[11]   The Sloan Digital Sky Survey photometric camera [J].
Gunn, JE ;
Carr, M ;
Rockosi, C ;
Sekiguchi, M ;
Berry, K ;
Elms, B ;
de Haas, E ;
Ivezic, Z ;
Knapp, G ;
Lupton, R ;
Pauls, G ;
Simcoe, R ;
Hirsch, R ;
Sanford, D ;
Wang, S ;
York, D ;
Harris, F ;
Annis, J ;
Bartozek, L ;
Boroski, W ;
Bakken, J ;
Haldeman, M ;
Kent, S ;
Holm, S ;
Holmgren, D ;
Petravick, D ;
Prosapio, A ;
Rechenmacher, R ;
Doi, M ;
Fukugita, M ;
Shimasaku, K ;
Okada, N ;
Hull, C ;
Siegmund, W ;
Mannery, E ;
Blouke, M ;
Heidtman, D ;
Schneider, D ;
Lucinio, R ;
Brinkman, J .
ASTRONOMICAL JOURNAL, 1998, 116 (06) :3040-3081
[12]  
KENNEFICK JD, 1995, AJ, V110, P255
[13]   A modified magnitude system that produces well-behaved magnitudes, colors, and errors even for low signal-to-noise ratio measurements [J].
Lupton, RH ;
Gunn, JE ;
Szalay, AS .
ASTRONOMICAL JOURNAL, 1999, 118 (03) :1406-1410
[14]  
LUPTON RH, 2000, UNPUB
[15]   The 3-53 keV spectrum of the quasar 1508+5714: X-rays from z=4.3 [J].
Moran, EC ;
Helfand, DJ .
ASTROPHYSICAL JOURNAL, 1997, 484 (02) :L95-L98
[16]   SECONDARY STANDARD STARS FOR ABSOLUTE SPECTROPHOTOMETRY [J].
OKE, JB ;
GUNN, JE .
ASTROPHYSICAL JOURNAL, 1983, 266 (02) :713-717
[17]   FAINT SPECTROPHOTOMETRIC STANDARD STARS [J].
OKE, JB .
ASTRONOMICAL JOURNAL, 1990, 99 (05) :1621-1631
[18]   Maps of dust infrared emission for use in estimation of reddening and cosmic microwave background radiation foregrounds [J].
Schlegel, DJ ;
Finkbeiner, DP ;
Davis, M .
ASTROPHYSICAL JOURNAL, 1998, 500 (02) :525-553
[19]   PC 1247+3406 - AN OPTICALLY SELECTED QUASAR WITH A REDSHIFT OF 4.897 [J].
SCHNEIDER, DP ;
SCHMIDT, M ;
GUNN, JE .
ASTRONOMICAL JOURNAL, 1991, 102 (03) :837-840
[20]   Four faint optically-selected quasars with redshifts greater than four [J].
Schneider, DP ;
Schmidt, M ;
Gunn, JE .
ASTRONOMICAL JOURNAL, 1997, 114 (01) :36-40