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Multiwavelength Mapping of Galaxy Formation and Evolution pp 434–435Cite as

The FORS Deep Field Spectroscopic Survey of High-Redshift Galaxies

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Part of the ESO Astrophysics Symposia book series (ESO)

Abstract

The evolution of the properties of galaxy populations with redshift provides important constraints on current models of galaxy formation and evolution. In order to investigate this evolution we used the FORS instruments at the VLT to obtain high-S/N galaxy spectra at redshifts up to 5.0 in the FORS Deep Field (FDF). A detailed discussion of the project can be found in [4].

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Authors and Affiliations

  1. Landessternwarte Königstuhl, 69117 Heidelberg, Germany

    Stefan Noll, Dörte Mehlert, Immo Appenzeller & Christian Tapken

Authors
  1. Stefan Noll
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  2. Dörte Mehlert
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  3. Immo Appenzeller
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  4. Christian Tapken
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Alvio Renzini Ralf Bender

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Noll, S., Mehlert, D., Appenzeller, I., Tapken, C. The FORS Deep Field Spectroscopic Survey of High-Redshift Galaxies. 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_96

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  • DOI: https://doi.org/10.1007/10995020_96

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  • 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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