Spectroscopy of quasar candidates from SDSS commissioning data
Author(s) -
Xiaohui Fan,
Michael A. Strauss,
J. Annis,
James E. Gunn,
G. S. Hennessy,
Željko Ivezić,
G. R. Knapp,
Robert H. Lupton,
Jeffrey A. Munn,
Heidi Jo Newberg,
Donald P. Schneider,
B. Yanny
Publication year - 1999
Publication title -
astrophysics
Language(s) - English
Resource type - Conference proceedings
DOI - 10.1063/1.58612
Subject(s) - quasar , redshift , sky , physics , astrophysics , astronomy , stars , spectroscopy , telescope , redshift survey , galaxy
The Sloan Digital Sky Survey has obtained images in five broad-band colorsfor several hundred square degrees. We present color-color diagrams for stellarobjects, and demonstrate that quasars are easily distinguished from stars bytheir distinctive colors. Follow-up spectroscopy in less than ten nights oftelescope time has yielded 22 new quasars, 9 of them at $z> 3.65$, and one with$z = 4.75$, the second highest-redshift quasar yet known. Roughly 80% of thehigh-redshift quasar candidates selected by color indeed turn out to behigh-redshift quasars.Comment: 4 pages, 3 figures, to appear in the proceedings of "After the Dark Ages: When Galaxies were Young (the Universe at 2
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom