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PC 1158 + 4635 - An optically selected quasar with a redshift of 4.73Photometric and spectroscopic observations of PC 1158 + 4635, a quasar with a redshift of 4.73, are presented. This object was discovered by the detection of its Ly-alpha emission line in a low-resolution CCD grism survey. The apparent magnitude of the quasar is r = 20.2; its absolute magnitude is similar to that of 3C 273 (for q0 = 0.5). The spectrum of PC 1158 + 4635 reveals prominent emission lines of Ly-alpha and C IV and a sharp, approximately one magnitude drop in the continuum level across the Ly-alpha emission line (features seen in most greater than 4 quasars). The redshift-continuum depression relation for quasars requires a dramatic change in the 'Lymann alpha clouds' (either in number or intrinsic properties) at a redshift of about 3.5 or else the presence of a new source that is responsible for the majority of the absorption at redshifts obove four.
Document ID
19900030471
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Schneider, Donald P.
(Institute for Advanced Study Princeton, NJ, United States)
Schmidt, Maarten
(Palomar Observatory Pasadena, CA, United States)
Gunn, James E.
(Princeton University Observatory, NJ, United States)
Date Acquired
August 14, 2013
Publication Date
December 1, 1989
Publication Information
Publication: Astronomical Journal
Volume: 98
ISSN: 0004-6256
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-6256
Accession Number
90A17526
Funding Number(s)
CONTRACT_GRANT: NAS5-29225
CONTRACT_GRANT: NSF AST-87-15508
CONTRACT_GRANT: NSF AST-86-18257-A2
Distribution Limits
Public
Copyright
Other

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