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Multiwavelength Mapping of Galaxy Formation and Evolution pp 347–348Cite as

Radio Properties of EROs in the Phoenix Deep Survey

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Part of the ESO Astrophysics Symposia book series (ESO)

Abstract

Insensitive to dust obscuration, radio wavelengths are ideal to study star-forming galaxies free of dust induced biases. Using data from the Phoenix Deep Survey, we have identified a sample of star-forming extremely red objects (EROs). Stacking of the radio images of the radio-undetected star-forming EROs revealed a significant radio detection. Using the expected median redshift, we estimate an average star-formation rate of 61 M⊙ yr–1 for these galaxies.

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Authors and Affiliations

  1. CAAUL, Observatory of Lisbon, Tapada da Ajuda, 1349-018 Lisbon, Portugal

    J. Afonso

  2. Dept. of Physics & Astronomy, University of Pittsburgh, 3941 O’Hara St, Pittsburgh, PA 15260, USA

    A.M. Hopkins

  3. Dept. of Astronomy and Astrophysics, University of Toronto, 60 St. George St, Toronto, Ontario M5S 3H8, Canada

    M. Sullivan

  4. ESA, STScI, 3700 San Martin Drive, Baltimore, MD 21218, USA

    B. Mobasher

  5. National Athens Observatory, I.Metaxa & Vas.Pavlou str., Athens 15236, Greece

    A. Georgakakis

  6. Australian Research Council, GPO Box 2702, Canberra, ACT 2601, Australia

    L.E. Cram

Authors
  1. J. Afonso
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  2. A.M. Hopkins
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  3. M. Sullivan
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  4. B. Mobasher
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  5. A. Georgakakis
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  6. L.E. Cram
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Alvio Renzini Ralf Bender

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Afonso, J., Hopkins, A., Sullivan, M., Mobasher, B., Georgakakis, A., Cram, L. Radio Properties of EROs in the Phoenix Deep Survey. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_54

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  • DOI: https://doi.org/10.1007/10995020_54

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-25665-6

  • Online ISBN: 978-3-540-31641-1

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

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