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Dusty Galaxies at the Highest Redshifts

Published online by Cambridge University Press:  17 August 2016

David L Clements ,
Josh Greenslade ,
Dominik A. Riechers ,
Julie Wardlow ,
Ismael Pérez-Fournon  and
The HerMES Red Collective, The HerMES & H-ATLAS Consortia
David L Clements
Affiliation:
Physics Department, Blackett Lab, Prince Consort Road, London SW7 2AZ, UK
Josh Greenslade
Affiliation:
Physics Department, Blackett Lab, Prince Consort Road, London SW7 2AZ, UK
Dominik A. Riechers
Affiliation:
Department of Astronomy, Cornell University, Space Sciences Building, Ithaca, NY 14853, USA
Julie Wardlow
Affiliation:
Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Denmark Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK
Ismael Pérez-Fournon
Affiliation:
Instituto de Astrofísica de Canarias, C/Vía Láctea, E-38200 La Laguna, Tenerife, Spain Departimento de Astrofísica, Universidad de La Laguna, E-38206, La Laguna, Tenerife, Spain
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Abstract

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The use of red colour as the basis for selecting candidate high redshift dusty galaxies from surveys made with Herschel has proved highly successful. The highest redshift such object, HFLS3, lies at z = 6.34 and numerous other sources have been found. Spectroscopic followup confirms that most of these lie at z > 4. These sources are found in such numbers that they represent a challenge to current models of galaxy evolution. We also examine the prospects for finding dusty galaxies at still higher redshifts. These would not appear in the SPIRE surveys from Herschel but would be detected in longer wavelength, submm, surveys. Several such ‘SPIRE-dropouts’ have been found and are now subject to followup observations.

Keywords

galaxies: starburstgalaxies: submmgalaxies:high redshift
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 84 - 87
Copyright
Copyright © International Astronomical Union 2016 

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