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Nine optically selected quasars with redshifts larger than 3The detection of nine quasars with redshifts between 3.0 and 3.8 is reported. The quasars were all found in a grism survey from their Lyman-alpha emission line. The r magnitudes of the quasars range from 18.5 to 21.7. The strengths of the Lyman-alpha lines are comparable to the values observed in other quasars (rest equivalent widths from 40 to 160 A). The spectrum of one of the objects possesses complex broad absorption features, similar to those seen in PHL 5200. A preliminary evaluation of these findings suggests that the comoving quasar density declines gradually beyond z = 3.
Document ID
19870052043
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Schmidt, Maarten
(Palomar Observatory Pasadena, CA, United States)
Schneider, Donald P.
(Institute for Advanced Study Princeton, NJ, United States)
Gunn, James E.
(Princeton University NJ, United States)
Date Acquired
August 13, 2013
Publication Date
May 1, 1987
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 316
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
87A39317
Funding Number(s)
CONTRACT_GRANT: NSF AST-83-14134
CONTRACT_GRANT: NSF AST-84-20352
CONTRACT_GRANT: NAS5-29225
Distribution Limits
Public
Copyright
Other

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