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A&A 442, 63-68 (2005)
DOI: 10.1051/0004-6361:20053365
Intergalactic HeII absorption towards QSO 1157+3143
D. Reimers1, C. Fechner1, H.-J. Hagen1, P. Jakobsen2, D. Tytler3 and D. Kirkman31 Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
e-mail: cfechner@hs.uni-hamburg.de
2 Astrophysics Missions Division, RSSD, European Space Agency, ESTEC, 2200 AG Noordwijk, The Netherlands
3 Center for Astrophysics and Space Sciences, University of California, San Diego, MS 0424, La Jolla, CA 92093-0424, USA
(Received 4 May 2005/ Accepted 30 June 2005 )
Abstract
We report the discovery of a further line of sight allowing detection
of
Ly
absorption by the intergalactic medium.
A HST/STIS survey of 32 bright
quasars selected from the Hamburg Quasar Surveys yielded one detection toward QSO 1157+3143 (
).
A 10 orbit follow-up spectrum reveals a UV spectrum significantly suppressed by two intervening Lyman limit systems at z=2.77 and 2.94, but with the
continuum flux recovering sufficiently shortward of ~
to allow study of the
absorption spectrum in the redshift range
.
The absorption is characterized by alternating voids and
dense filament structures seen in both
and
.
Attempts to model the
opacity in terms of
Ly
forest absorption are not successful in the voids, suggesting that
reionization is not complete between z=2.77 and 2.97 or that an optically thin Lyman limit system with
is responsible for the additional opacity.
Key words: galaxies: quasars: individual: QSO 1157+3143 -- galaxies: quasars: absorption lines -- cosmology: observations
SIMBAD Objects
© ESO 2005
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