Overview
- Editors:
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Raffaella Morganti
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Istituto di Radioastronomia, Bologna, Italy
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Warrick J. Couch
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School of Physics, University of New South Wales, Sydney, Australia
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Table of contents (65 papers)
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Coordinating Multi-Wavelength Observations
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- Roger W. Clay, Bruce R. Dawson
Pages 199-200
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- Michael G. Burton, John W. V. Storey, Michael C. B. Ashley
Pages 201-208
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The High-Redshift Universe
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Front Matter
Pages 209-209
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- I. M. Hook, R G. McMahon, P. A. Shaver
Pages 211-215
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- F. La Franca, P. Andreani, S. Cristiani
Pages 216-220
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- Jochen Liske, John K. Webb
Pages 234-235
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- Wil van Breugel, Carlos De Breuck, Huub Röttgering, George Miley, Adam Stanford
Pages 236-245
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- Carlos De Breuck, Wil van Breugel, Huub Röttgering, George Miley, Chris Carilli
Pages 246-247
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- Z. Tsvetanov, R. Morganti, R. A. E. Fosbury, M. G. Allen, J. Gallimore
Pages 248-249
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- Alberto Fernández-Soto, Kenneth M. Lanzetta, Amos Yahil
Pages 270-274
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- Katrina Sealey, Michael Drinkwater, John Webb, Brian Boyle
Pages 278-279
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- Brigitte Rocca-Volmerange, Michel Fioc
Pages 289-293
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About this book
The idea of a joint ESO / Australia meeting on the large number of exciting new facilities that are, or will soon be, available tihne southern hemisphere arose quite naturally. In the optical and the near-infrared, the Very Large Telescope (VLT) will soon be operational. In the radio, the Australia Telescope Com pact Array is going to be upgraded to higher frequencies (20 and 100 GHz), together with an improvement in very long baseline interferometry (VLBI) facil ities. Other major facilities, such as the Large Millimetre Array and the lkT are being planned. Moreover, new deep surveys are underway in the southern hemi sphere: the southern Hubble Deep Field, the ESO Imaging Survey (BIS), pan oramic deep surveys with the UK Schmidt telescope, and the Anglo-Australian Telescope (AAT) 2dF galaxy/QSO redshift survey in the optical; and the Parkes multibeam HI survey and Molonglo Observatory Synthesis Telescope (MOST) Wide Field continuum survey at radio wavelengths. With all these new facilities, important progress will be made regarding important issues such as the large scale structure of the universe, the very early universe and the associated first epoch of galaxy formation. The generation of large databases, and the oppor tunity for sensitive follow-up observations in complementary wavebands, mean that coordinated radio, infrared and optical projects in the southern hemisphere are likely to become increasingly attractive and important.
Editors and Affiliations
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Istituto di Radioastronomia, Bologna, Italy
Raffaella Morganti
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School of Physics, University of New South Wales, Sydney, Australia
Warrick J. Couch