| Literature DB >> 29769675 |
Takuya Hashimoto1,2, Nicolas Laporte3,4, Ken Mawatari5, Richard S Ellis3, Akio K Inoue5, Erik Zackrisson6, Guido Roberts-Borsani3, Wei Zheng7, Yoichi Tamura8, Franz E Bauer9,10,11, Thomas Fletcher3, Yuichi Harikane12,13, Bunyo Hatsukade14, Natsuki H Hayatsu13,15, Yuichi Matsuda16,17, Hiroshi Matsuo16,17, Takashi Okamoto18, Masami Ouchi12,19, Roser Pelló4, Claes-Erik Rydberg20, Ikkoh Shimizu21, Yoshiaki Taniguchi22, Hideki Umehata14,22,23, Naoki Yoshida13,19.
Abstract
A fundamental quest of modern astronomy is to locate the earliest galaxies and study how they influenced the intergalactic medium a few hundred million years after the Big Bang1-3. The abundance of star-forming galaxies is known to decline4,5 from redshifts of about 6 to 10, but a key question is the extent of star formation at even earlier times, corresponding to the period when the first galaxies might have emerged. Here we report spectroscopic observations of MACS1149-JD1 6 , a gravitationally lensed galaxy observed when the Universe was less than four per cent of its present age. We detect an emission line of doubly ionized oxygen at a redshift of 9.1096 ± 0.0006, with an uncertainty of one standard deviation. This precisely determined redshift indicates that the red rest-frame optical colour arises from a dominant stellar component that formed about 250 million years after the Big Bang, corresponding to a redshift of about 15. Our results indicate that it may be possible to detect such early episodes of star formation in similar galaxies with future telescopes.Entities:
Year: 2018 PMID: 29769675 DOI: 10.1038/s41586-018-0117-z
Source DB: PubMed Journal: Nature ISSN: 0028-0836 Impact factor: 49.962