Volume 442, Number 1, October IV 2005
|Page(s)||63 - 68|
|Section||Cosmology (including clusters of galaxies)|
|Published online||30 September 2005|
Intergalactic HeII absorption towards QSO 1157+3143
Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany e-mail: firstname.lastname@example.org
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
Accepted: 30 June 2005
We report the discovery of a further line of sight allowing detection of Lyα 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 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 Lyα forest absorption are not successful in the voids, suggesting that reionization is not complete between 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
© ESO, 2005
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