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The Discovery of a High-Redshift Quasar without Emission Lines from Sloan Digital Sky Survey Commissioning Data
Author(s) -
Xiaohui Fan,
Michael A. Strauss,
James E. Gunn,
Robert H. Lupton,
C. L. Carilli,
M. P. Rupen,
Gary D. Schmidt,
Leonidas A. Moustakas,
Marc Davis,
James Annis,
Neta A. Bahcall,
J. Brinkmann,
Róbert Brunner,
István Csabai,
Mamoru Doi,
M. Fukugita,
Timothy M. Heckman,
G. S. Hennessy,
Robert B. Hindsley,
Željko Ivezić,
G. R. Knapp,
D. Q. Lamb,
Jeffrey A. Munn,
A. George Pauls,
Jeffrey R. Pier,
Constance M. Rockosi,
Donald P. Schneider,
Alexander S. Szalay,
D. L. Tucker,
Donald G. York
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/312382
Subject(s) - astrophysics , physics , quasar , redshift , galaxy , sky , bl lac object , astronomy , emission spectrum , flux (metallurgy) , redshift survey , x shaped radio galaxy , spectral line , blazar , gamma ray , materials science , metallurgy
We report observations of a luminous unresolved object at redshift z=4.62, with a featureless optical spectrum redward of the Lyalpha forest region, discovered from Sloan Digital Sky Survey commissioning data. The redshift is determined by the onset of the Lyalpha forest at lambda approximately 6800 Å and a Lyman limit system at lambda=5120 Å. A strong Lyalpha absorption system with weak metal absorption lines at z=4.58 is also identified in the spectrum. The object has a continuum absolute magnitude of -26.6 at 1450 Å in the rest frame (h0=0.5, q0=0.5) and therefore cannot be an ordinary galaxy. It shows no radio emission (the 3 sigma upper limit of its flux at 6 cm is 60 µJy), indicating a radio-to-optical flux ratio at least as small as that of the radio-weakest BL Lacertae objects known. It is also not linearly polarized to a 3 sigma upper limit of 4% in the observed I band. Therefore, it is either the most distant BL Lac object known to date, with very weak radio emission, or a new type of unbeamed quasar, whose broad emission line region is very weak or absent.

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