The Square Kilometre Array: Paving the way for the new 21st century radio astronomy paradigm

Proceedings of Symposium 7 of JENAM 2010

  • Domingos Barbosa
  • Sonia Anton
  • Leonid Gurvits
  • Dalmiro Maia

Part of the Astrophysics and Space Science Proceedings book series (ASSSP)

Table of contents

  1. Front Matter
    Pages i-x
  2. David R. DeBoer
    Pages 1-8
  3. A. van Ardenne, A. J. Faulkner, J. G. bij de Vaate
    Pages 9-15
  4. Paolo Padovani
    Pages 17-30
  5. W. J. G. de Blok, S.-H. Oh, B. S. Frank
    Pages 43-51
  6. A. P. Lobanov
    Pages 75-83
  7. L. Bizzocchi, J. Afonso, E. Ibar, M. Grossi, C. Simpson, S. Chapman et al.
    Pages 97-100
  8. M. B. Silva, M. G. Santos, J. R. Pritchard, R. Cen, A. Cooray
    Pages 101-116

About these proceedings

Introduction

The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telescope over a wavelength range of several hundred to one, from decametric to microwave wavelengths. It will revolutionize the study of the most abundant element in the Universe, hydrogen, from the epoch of reionisation to the present-day, probing the onset formation period of the very first stars, will closely scan proto-planets and, through the precision timing of pulsars, will detect the distortions of space-time due to gravitational radiation. The SKA is a sensing network spanning 3000 km from its centre and with a collecting area of more than 1 square kilometre, using technologies of the 21st century. The SKA will make the study of a wide range of phenomena initially studied at other wavelengths possible at radio wavelengths, as well as opening a new discovery window on new phenomena at radio wavelengths.
Symposium 7 of the JENAM 2010 aimed at bringing these diverse opportunities to the attention of both theoretical and observational astronomers working at all wavelengths, including the potential for synergies with other facilities. The meeting


·        highlighted the scientific potential of the SKA
·        discussed  scientific priorities and their impact on the design of the SKA
·        explored the synergies between the SKA and other next-generation astronomical facilities in different wavelength domains such as the ALMA, ELTs, LSST, JWST, GRE, IXO, Gaia and Euclid, and high-energy facilities (Auger)
·        explored the “cyber–infrastructure” that may become available for the distribution and distributed analysis of SKA data

Keywords

Radio astronomy in 21st century SKA Square Kilometre Array

Editors and affiliations

  • Domingos Barbosa
    • 1
  • Sonia Anton
    • 2
  • Leonid Gurvits
    • 3
  • Dalmiro Maia
    • 4
  1. 1., Telecomunicações, Campus Univ. de AveiroRadio Astronomy Group, Instituto deAveiroPortugal
  2. 2., Departamento de MatemáticaCICGEPortoPortugal
  3. 3.Joint Institute for VLBI in EuropeDwingelooNetherlands
  4. 4., Observatorio Astronomico Manuel de BarroCICGE-UPVila Nova de GaiaPortugal

Bibliographic information

  • DOI https://doi.org/10.1007/978-3-642-22795-0
  • Copyright Information Springer-Verlag Berlin Heidelberg 2012
  • Publisher Name Springer, Berlin, Heidelberg
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-3-642-22794-3
  • Online ISBN 978-3-642-22795-0
  • Series Print ISSN 1570-6591
  • Series Online ISSN 1570-6605
  • About this book
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