We report the discovery of a further line of sight allowing detection of He II Lyα 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 suppressed by two intervening Lyman limit systems at z = 2.77 and 2.94, but with the continuum flux recovering sufficiently shortward of ∼ 1700 Å to allow study of the He II 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 He II and H I. Attempts to model the He II opacity in terms of HI Lyα forest absorption are not successful in the voids, suggesting that He II 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. © ESO 2005.
CITATION STYLE
Reimers, D., Fechner, C., Hagen, H. J., Jakobsen, P., Tytler, D., & Kirkman, D. (2005). Intergalactic Hell absorption towards QSO 1157+3143. Astronomy and Astrophysics, 442(1), 63–68. https://doi.org/10.1051/0004-6361:20053365
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