Near-infrared colors of gamma-ray burst afterglows and cosmic reionization history

Akio K. Indue*, Ryo Yamazaki, Takashi Nakamura

*この研究の対応する著者

研究成果: Article査読

11 被引用数 (Scopus)

抄録

We discuss a way to study the cosmic reionization history using near-infrared (NIR) observations of the afterglows of high-redshift (5 ≲ z ≲ 25) gamma-ray bursts (GRBs) that will be detected by the Swift satellite. In principle, details of the cosmic reionization history should be imprinted in the NIR spectra of GRB afterglows. However, spectroscopy with a space telescope is required to obtain such information for very high redshifts (z ≳ 15) unless the neutral fraction of the high-z universe is less than 10-6. The broadband photometry has higher sensitivity than the spectroscopy, so that NIR photometric follow-up of GRB afterglows is very promising for examining cosmic reionization history. A few minutes exposure with a 8 m class ground-based telescope of the afterglows of the high-z GRBs will reveal how many times reionization occurred in the universe.

本文言語English
ページ(範囲)644-653
ページ数10
ジャーナルAstrophysical Journal
601
2 I
DOI
出版ステータスPublished - 2004 2 1
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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