A dusty, normal galaxy in the epoch of reionization

Darach Watson (), Lise Christensen, Kirsten Kraiberg Knudsen, Johan Richard, Anna Gallazzi and Michał Jerzy Michałowski
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Darach Watson: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 32, København Ø, 2100, Denmark
Lise Christensen: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 32, København Ø, 2100, Denmark
Kirsten Kraiberg Knudsen: Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden
Johan Richard: Centre de Recherche Astrophysique de Lyon, Observatoire de Lyon, Université Lyon 1, 9 Avenue Charles André, 69561 Saint Genis Laval Cedex, France
Anna Gallazzi: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 32, København Ø, 2100, Denmark
Michał Jerzy Michałowski: The Scottish Universities Physics Alliance, Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ, UK

Nature, 2015, vol. 519, issue 7543, 327-330

Abstract: Far-infrared measurements of galaxies in the early Universe would reveal their detailed properties, but have been lacking for the more typical galaxies where most stars form; here an archetypal, early Universe star-forming galaxy is detected at far-infrared wavelengths, allowing its dust mass, total star-formation rate and dust-to-gas ratio to be calculated.

Date: 2015
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DOI: 10.1038/nature14164

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