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A study of ten quasars with redshifts greater than fourFour quasars with redshifts greater than four were detected in a low-resolution CCD grism survey. CCD photometry and high S/N, moderate resolution spectra are presented for these quasars and the six other known quasars with redshifts above 4. The M sub B values of nine of the objects are between -27.5 and -25, with the tenth quasar having an M sub B value of -29. The emission lines and shapes of the continua of these ten quasars are similar to those of lower-redshift quasars. The results suggest that the C IV emission lines in high-redshift quasars may be weaker than those in lower-redshift quasars. The continua of all of the high-redshift quasars display strong depressions blueward of the Ly-alpha emission line.
Document ID
19900027176
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
November 1, 1989
Publication Information
Publication: Astronomical Journal
Volume: 98
ISSN: 0004-6256
Subject Category
Astrophysics
Accession Number
90A14231
Funding Number(s)
CONTRACT_GRANT: NSF AST-86-18257
CONTRACT_GRANT: NSF AST-87-15508
CONTRACT_GRANT: NAS5-29225
Distribution Limits
Public
Copyright
Other

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