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Multiwavelength Observations of the Subaru/XMM-Newton Deep Field

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Multiwavelength Mapping of Galaxy Formation and Evolution

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

Abstract

The Subaru/XMM-Newton Deep Survey (SXDS) is a new deep Optical/X-ray survey, whose purpose is to provide an accurate census of the contents of the Universe without suffering from the biasing effects of large-scale structures. The SXDS is part of an ambitious project to obtain extensive multi-wavelength data across a ~1.3 deg2 region of sky. Other wavelength observations ranging from the X-ray to the radio are being pursued and/or planned through various facilities. These multiwavelength data would allow us a comprehensive approach to investigate the mass assembly history of galaxies over a broad span of cosmic history.

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Alvio Renzini Ralf Bender

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Sekiguchi, K. et al. Multiwavelength Observations of the Subaru/XMM-Newton Deep Field. 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_12

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  • DOI: https://doi.org/10.1007/10995020_12

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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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