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arXiv · astro-ph/0609393

A galaxy at a redshift z = 6.96

Masanori Iye·Kazuaki Ota·Nobunari Kashikawa·Hisanori Furusawa·Tetsuya Hashimoto·Takashi Hattori·Yuichi Matsuda·Tomoki Morokuma·Masami Ouchi·Kazuhiro Shimasaku
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Abstract

When galaxy formation started in the history of the Universe remains unclear. Studies of the cosmic microwave background indicate that the Universe, after initial cooling (following the Big Bang), was reheated and reionized by hot stars in newborn galaxies at a redshift in the range 6 < z < 14 (ref. 1). Though several candidate galaxies at redshift z > 7 have been identified photometrically (refs 2,3), galaxies with spectroscopically confirmed redshifts have been confined to z < 6.6 (refs. 4-8). Here we report a spectroscopic redshift of z = 6.96 (corresponding to just 750 Myr after the Big Bang) for a galaxy whose spectrum clearly shows Lyman-alpha emission at 9,682 A, indicating active star formation at a rate of about 10 M_sun/yr, where M_sun us the mass of the Sun. This demonstrates that galaxy formation was under way when the Universe was only about 6 per cent of its present age. The number density of galaxies at z = 7 seems to be only 18-36 per cent of the density at z = 6.6.

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Masanori Iye, Kazuaki Ota, Nobunari Kashikawa, Hisanori Furusawa, Tetsuya Hashimoto, Takashi Hattori, Yuichi Matsuda, Tomoki Morokuma, Masami Ouchi, Kazuhiro Shimasaku. 2006-09-14. A galaxy at a redshift z = 6.96. https://doi.org/10.1038/nature05104

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