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A dusty, normal galaxy in the epoch of reionization

Author

Listed:
  • 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
    Istituto Nazionale di Astrofisica-Osservatorio Astrosico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy)

  • Michał Jerzy Michałowski

    (The Scottish Universities Physics Alliance, Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ, UK)

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.

Suggested Citation

  • Darach Watson & Lise Christensen & Kirsten Kraiberg Knudsen & Johan Richard & Anna Gallazzi & Michał Jerzy Michałowski, 2015. "A dusty, normal galaxy in the epoch of reionization," Nature, Nature, vol. 519(7543), pages 327-330, March.
    • Handle: RePEc:nat:nature:v:519:y:2015:i:7543:d:10.1038_nature14164
    DOI: 10.1038/nature14164
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