Intergalactic HeII absorption towards QSO 1157+3143
arXiv:astro-ph/0507178 · doi:10.1051/0004-6361:20053365
Abstract
We report the discovery of a further line of sight allowing detection of HeII Ly alpha absorption by the intergalactic medium. A HST/STIS survey of 32 bright z ~ 3 quasars selected from the Hamburg Quasar Surveys yielded one detection toward QSO 1157+3143 (z ~ 3, B ~ 17). A 10 orbit follow-up spectrum reveals a UV spectrum significantly supressed by two intervening Lyman limit systems at z=2.77 and 2.94, but with the continuum flux recovering sufficiently shortward of ~ 1700 A to allow study of the HeII absorption spectrum in the redshift range 2.75 < z < 2.97. The absorption is characterized by alternating voids and dense filament structures seen in both HeII and HI. Attempts to model the HeII opacity in terms of HI Ly alpha forest absorption are not successful in the voids, suggesting that HeII reionization is not complete between z=2.77 and 2.97 or that an optically thin Lyman limit system with z ~ 0.3 is responsible for the additional opacity.
6 pages, 4 figures, accepted by A&A
References in corpus (8)
- The thermal history of the intergalactic medium
- The Evolution of the Effective Equation of State of the IGM
- Constraints on reionization from the thermal history of the intergalactic medium
- Resolving the Structure of Ionized Helium in the Intergalactic Medium with the Far Ultraviolet Spectroscopic Explorer
- The Fluctuating Intergalactic Radiation Field at Redshifts z = 2.3-2.9 from He II and H I Absorption towards HE 2347-4342
- Caught in the act: a helium-reionizing quasar near the line of sight to Q0302-003
- Detection of Intergalactic HeII Absorption at Redshift 3.5
- The Absorbers Toward CSO 118: Superclustering at {z~3}, or an Intrinsic Absorption Complex?
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