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High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data. II. The Spring Equatorial Stripe
Author(s) -
Xiaohui Fan,
Michael A. Strauss,
Donald P. Schneider,
James E. Gunn,
Robert H. Lupton,
Scott F. Anderson,
W. Voges,
B. Margon,
James Annis,
Neta A. Bahcall,
J. Brinkmann,
Róbert Brunner,
Michael A. Carr,
István Csabai,
Mamoru Doi,
Joshua A. Frieman,
M. Fukugita,
G. S. Hennessy,
Robert B. Hindsley,
Željko Ivezić,
G. R. Knapp,
D. Q. Lamb,
Timothy A. McKay,
Jeffrey A. Munn,
Heidi Jo Newberg,
A. George Pauls,
Jeffrey R. Pier,
R. Rechenmacher,
Gordon T. Richards,
Constance M. Rockosi,
Chris Stoughton,
Alexander S. Szalay,
Aniruddha R. Thakar,
D. L. Tucker,
Patrick Waddell,
Donald G. York
Publication year - 2000
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/301191
Subject(s) - quasar , redshift , astrophysics , physics , sky , photometry (optics) , astronomy , emission spectrum , ovv quasar , absolute magnitude , spectral line , stars , galaxy
This is the second paper in a series aimed at finding high-redshift quasarsfrom five-color (u'g'r'i'z') imaging data taken along the Celestial Equator bythe Sloan Digital Sky Survey (SDSS) during its commissioning phase. In thispaper, we present 22 high-redshift quasars (z>3.6) discovered from ~250 deg^2of data in the spring Equatorial Stripe, plus photometry for two previouslyknown high-redshift quasars in the same region of sky. Our success rate ofidentifying high-redshift quasars is 68%. Five of the newly discovered quasarshave redshifts higher than 4.6 (z=4.62, 4.69, 4.70, 4.92 and 5.03). All thequasars have i* < 20.2 with absolute magnitude -28.8 < M_B < -26.1 (h=0.5,q_0=0.5). Several of the quasars show unusual emission and absorption featuresin their spectra, including an object at z=4.62 without detectable emissionlines, and a Broad Absorption Line (BAL) quasar at z=4.92.

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