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The MUNICS Project: Galaxy Assembly at 0 < z < 1

  • Conference paper
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Multiwavelength Mapping of Galaxy Formation and Evolution

Part of the book series: ESO Astrophysics Symposia ((ESO))

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Abstract

MUNICS is a wide-area, medium-deep, photometric and spectroscopic survey selected in the K band, targeting randomly-selected high Galactic latitude fields. It covers an area of roughly one square degree in the K and J bands with complementary optical follow-up imaging in the I, R, V, and B bands in 0.5 square degrees.

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Authors and Affiliations

  1. University of Texas at Austin, Austin, TX 78712, USA

    Niv Drory & Gary J. Hill

  2. Max–Planck Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching bei München, Germany

    Ralf Bender & Claudia Maraston

  3. Universitäts-Sternwarte München, Scheinerstraße 1, 81679 München, Germany

    Ralf Bender, Georg Feulner, Ulrich Hopp & Jan Snigula

Authors
  1. Niv Drory
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  2. Ralf Bender
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  3. Georg Feulner
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  4. Gary J. Hill
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  5. Ulrich Hopp
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  6. Claudia Maraston
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  7. Jan Snigula
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Editor information

Alvio Renzini Ralf Bender

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Drory, N. et al. The MUNICS Project: Galaxy Assembly at 0 < z < 1. 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_38

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  • DOI: https://doi.org/10.1007/10995020_38

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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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