Evolution of Large-Scale Structure:
From Recombination to Garching
August 2-7 1998
The meeting covered current observational and theoretical research on the large-scale structure of the Universe. It took a broad view, exploring connections between cosmic microwave background fluctuations, high-redshift structure in the intergalactic medium and galaxy distribution, and the present-day distribution of galaxies and dark matter. Review speakers gave overviews of the present state of the field, as well as indicating where significant new developments were likely to occur. Targetted talks presented the most exciting results of the last year or two. There were also opportunities for participants to contribute shorter talks and posters.
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Invited Reviewers:
M. Bartelmann, S. Cristiani, L. da Costa, A. Evrard, C. Lawrence, J. Peacock, M. Postman, C. Steidel, M. Strauss, N. Sugiyama, A. Szalay, D. Weinberg
Topics covered:
Cosmic Microwave Background, Gravitational Lensing, Redshift Surveys, Peculiar Velocity Studies, Models and Measures of Clustering, High-redshift Universe, Numerical Simulations
J. Bergeron (ESO, Garching), M. Davis (UC, Berkeley), A. Dekel (HU, Jerusalem), K. M. Gorski (TAC, Copenhagen), J. Silk (UC, Berkeley), R. Sunyaev (MPA, Garching), and A. Szalay (JHU, Baltimore).
A. J. Banday, M. Bartelmann, H. Mo, A. Nusser, R. K. Sheth,
S. D. M. White (MPA)
L. da Costa, A. Renzini (ESO)
For further information please contact:
cosmo@mpa-garching.mpg.de
List of Participants |
Timetable |
Abstracts for oral presentations |
Poster presentations |
Outline of topics to be covered |
Map of Garching |
Travel Information |
Accommodation |
Guidelines for proceedings |
On-line
Proceedings |
Acknowledgements: NTT SUSI Deep Field courtesy D'Odorico et al. 1998.