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Lyman Alpha Emitting and Related Star-Forming Galaxies at High Redshift

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Lessons from the Local Group

Abstract

I provide an overview about star-forming galaxies at high redshift and their physical properties. Starting from the populations of Lyα emitters and Lyman break galaxies, I summarize their common features and distinction. Then I summarize recent insight onto their physical properties gained from SED models including nebular emission, and various implications from these studies on the properties of star-formation at high redshift. Finally, I present new results and an overview on the dust content and UV attenuation of \(z>6\) galaxies obtained from IRAM and ALMA observations.

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Acknowledgements

I wish to warmly thank the organizers, David Block, Ken Freeman, and Bruce Elmegreen for this very interesting and exceptional meeting. I thank my collaborators, in particular Anne Verhamme, Frederic Boone, Mirka Dessauges, Michel Zamojski, Stephane de Barros, and Panos Sklias for their contributions to some of the work presented here.

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Authors and Affiliations

  1. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290, Versoix, Switzerland

    Daniel Schaerer

  2. IRAP, CNRS, 14 Avenue E. Belin, 31400, Toulouse, France

    Daniel Schaerer

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  1. Daniel Schaerer
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Correspondence to Daniel Schaerer .

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Editors and Affiliations

  1. Australian National University, Canberra, Australia

    Kenneth Freeman

  2. IBM T.J. Watson Research Center, Yorktown Heights, New York, USA

    Bruce Elmegreen

  3. University of the Witwatersrand, Johannesburg, South Africa

    David Block

  4. University of the Witwatersrand, Johannesburg, South Africa

    Matthew Woolway

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Schaerer, D. (2015). Lyman Alpha Emitting and Related Star-Forming Galaxies at High Redshift. In: Freeman, K., Elmegreen, B., Block, D., Woolway, M. (eds) Lessons from the Local Group. Springer, Cham. https://doi.org/10.1007/978-3-319-10614-4_38

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