Rencontres de Moriond
Very High Energy Phenomena in the Universe
La Thuile, Italy (March 12-19, 2005)
A composite Chandra X-ray (blue) and Palomar infrared (red and green) image of the supernova remnant W49B. Credit: X-ray: NASA/Chandra X-ray Center/Spitzer Science Center; Infrared: Caltech/Palomar
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- Ultra High Energy Cosmic Rays
- Origin and Propagation of CR
- High Energy Gamma Ray Astronomy
- Compact objects
- Gamma Ray Bursts
- Neutrino astrophysics
- Dark Matter, Extra dimension physics
Scientific Program (agenda and link to the transparencies)
Program Committee :
R. Ansari (Orsay),
M. Boratav (Paris),
G. Bogaert (Palaiseau),
S. Collin (Meudon),
J. Dumarchez (Paris),
Y. Giraud-Héraud (Paris),
C. Magneville (Saclay),
E. Parizot (Orsay),
E. Plagnol (Paris),
G. Sigl (Paris),
H. Sol (Meudon),
J. Trân Thanh Vân (Orsay),
You can find more organizational details in the
Bulletin Nr 1
Registration is closed
Accommodation Grants
Partial support from the European Union "Marie Curie" Program
is available for a limited number of scientists.
Proceedings
The deadline for sending the manuscripts is: May 15, 2005
The proceedings will be available during summer.
The speakers have to use the following 2 files to prepare the written version
of their talk under Latex:
moriond.tex (containing the publisher's instruction: it can be used as
a template. The result can be visualised on
moriond.ps),
and
moriond.sty (the style file).
The speakers should send their written contribution
to Jacques.Dumarchez@cern.ch
(possibly as a .tar.gz file - compressed tar)
In case of problems with Latex send a mail to Jacques.Dumarchez@cern.ch.
Secretariat:
Mrs Elizabeth Hautefeuille
Rencontres de Moriond, BP 33
104, avenue du Général Leclerc
F-91192 GIF SUR YVETTE CEDEX , France
Phone : (33 1) 69 29 05 50 Fax : (33 1) 69 28 86 59
E-mail : elizabeth.hautefeuille@th.u-psud.fr
http://moriond.in2p3.fr/J05/
Sponsors:
CNRS - IN2P3, CEA-DAPNIA, NSF, EU
Jacques Dumarchez
Last modified: Tue Nov 23 16:57:40 MET