z-logo
open-access-imgOpen Access
How Universal is the Gunn-Peterson Trough at z ~ 6?: A Closer Look at the Quasar SDSS J1148+5251
Author(s) -
S. Peng Oh,
Steven R. Furlanetto
Publication year - 2005
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 - 10.1086/428610
Subject(s) - quasar , astrophysics , physics , redshift , cosmic variance , galaxy , intergalactic travel , astronomy , trough (economics) , flux (metallurgy) , optical depth , chemistry , meteorology , aerosol , economics , macroeconomics , organic chemistry
Detectable flux is visible in the Ly-alpha and Ly-beta troughs of the highestredshift ($z=6.42$) quasar found to date, SDSS J1148+5251. This has previouslybeen interpreted as continuum contamination from an interloper galaxy atz=4.94. We examine the Ly-gamma trough of SDSS J1148+5251 and show that thisinterpretation is untenable: the spectrum does not show the continuum break ina z=4.94 galaxy expected from absorption by the intervening Ly-alpha forest.Therefore, flux must be leaking through at least one of the troughs from thequasar itself. Contrary to previous claims, the flux ratios in the Ly-alpha andLy-beta troughs are consistent with pure transmission. From the Ly-gammatrough, we place an upper bound on the effective Ly-alpha optical depth atz~6.2 of tau < 14.3 (2 sigma). This implies a highly ionized IGM along thisline of sight and significant cosmic variance in the transition toward completeGunn-Peterson absorption. Detailed study of the observed transmission featureswill shed light on this era.Comment: Submitted to ApJ Letter

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom