Detection of intergalactic He II absorption at redshift 3.5

Wei Zheng, Kuenley Chiu, Scott F. Anderson, Donald P. Schneider, Craig J. Hogan, Donald G. York, Scott Burles, Jonathan Brinkmann

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Abstract

The large number of quasars found in the Sloan Digital Sky Survey has allowed searches for elusive, clear lines of sight toward He II Lyα absorption, a sensitive probe of the intergalactic medium. The few known systems indicate that He II reionization occurs at z > 3. We report the detection of a He II Lyα absorption edge in a quasar spectrum at z = 3.50, the most distant such feature found to date. The candidate quasar was selected from a z ∼ 3 sample in the Sloan Digital Sky Survey spectroscopic quasar survey and confirmed as part of an HST Space Telescope Imaging Spectrograph SNAP survey. We discuss the general characteristics of the absorption feature, as well as the probability for the discovery of additional such objects.

Original languageEnglish (US)
Pages (from-to)656-659
Number of pages4
JournalAstronomical Journal
Volume127
Issue number2 1778
DOIs
StatePublished - Feb 1 2004

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All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Zheng, W., Chiu, K., Anderson, S. F., Schneider, D. P., Hogan, C. J., York, D. G., Burles, S., & Brinkmann, J. (2004). Detection of intergalactic He II absorption at redshift 3.5. Astronomical Journal, 127(2 1778), 656-659. https://doi.org/10.1086/381485