An updated analytic model for attenuation by the intergalactic medium

Akio K. Inoue*, Ikkoh Shimizu, Ikuru Iwata, Masayuki Tanaka

*この研究の対応する著者

研究成果: Article査読

184 被引用数 (Scopus)

抄録

We present an updated version of the so-called Madau model for attenuation of the radiation from distant objects by intergalactic neutral hydrogen. First, we derive the distribution function of intergalactic absorbers from the latest observational statistics of the Lyα forest, Lymanlimit systems and damped Lyα systems. The distribution function reproduces the observed redshift evolution of the Lyα depression and the mean-free path of the Lyman continuum excellently and simultaneously. We then derive a set of analytic functions describing the mean intergalactic attenuation curve for objects at z > 0.5. The new model predicts less (or more) Lyα attenuation for z ≃ 3-5 (z > 6) sources through the usual broad-band filters relative to the original Madau model. This may cause a systematic difference in the photometric redshift estimates, which is, however, still small: about 0.05. Finally, we find a more than 0.5 mag overestimation of Lyman-continuum attenuation in the original Madau model at z > 3, which causes a significant overcorrection against direct observations of the Lyman continuum of galaxies.

本文言語English
ページ(範囲)1805-1820
ページ数16
ジャーナルMonthly Notices of the Royal Astronomical Society
442
2
DOI
出版ステータスPublished - 2014 6月
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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