A dominant population of optically invisible massive galaxies in the early Universe

Nature
T WangW-H Wang

Abstract

Our current knowledge of cosmic star-formation history during the first two billion years (corresponding to redshift z > 3) is mainly based on galaxies identified in rest-frame ultraviolet light1. However, this population of galaxies is known to under-represent the most massive galaxies, which have rich dust content and/or old stellar populations. This raises the questions of the true abundance of massive galaxies and the star-formation-rate density in the early Universe. Although several massive galaxies that are invisible in the ultraviolet have recently been confirmed at early epochs2-4, most of them are extreme starburst galaxies with star-formation rates exceeding 1,000 solar masses per year, suggesting that they are unlikely to represent the bulk population of massive galaxies. Here we report submillimetre (wavelength 870 micrometres) detections of 39 massive star-forming galaxies at z > 3, which are unseen in the spectral region from the deepest ultraviolet to the near-infrared. With a space density of about 2 × 10-5 per cubic megaparsec (two orders of magnitude higher than extreme starbursts5) and star-formation rates of 200 solar masses per year, these galaxies represent the bulk population of massive galaxies that has...Continue Reading

References

Apr 20, 2013·Nature·Dominik A RiechersJ Zmuidzinas
Apr 7, 2017·Nature·Karl GlazebrookTiantian Yuan

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Citations

Jan 26, 2021·Royal Society Open Science·J A Hodge, E da Cunha

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Software Mentioned

GaBoDS
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