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News: The congress photos are now available on "Photos" web page
"The Extreme sky:
Sampling the Universe above 10 keV"
13th - 17th October 2009
Otranto (Lecce) Italy,
Castello Aragonese
All-sky
surveys form the foundation of observational astronomy as they provide
With
respect to other surveys, those at high energies (above 10 keV) are
particularly interesting as they probe the energy domain where
fundamental changes from thermal to non-thermal sources/phenomena are
expected, where the effects of absorption are drastically reduced, and a
clearer picture of the Universe is possible. This is also the energy
range where most of the extreme astrophysical behaviour is taking place,
e.g. cosmic acceleration, explosions and accretion onto black holes and
neutron stars. Recently a number of surveys have been performed in the
keV to TeV energy range.
The
objective of this workshop is to gather all the knowledge collected so
far above 10 keV, to compare and contrast the results obtained in the
various bands in the light of physical models and ultimately provide
indications for future progress. The meeting is aimed at bringing
together scientists active across the high energy range in order to
focus on the opportunities offered by this new window both from the
observational and theoretical viewpoints, while a dedicated section will
also be devoted to discuss future mission ideas. The meeting will
consist of invited talks and contributions which are welcome as either
posters or as short interventions. There will be time for open
discussions throughout. Finally, this meeting is a perfect way in which
to celebrate with friends and colleagues INTEGRAL's 7th birthday and 7
years of success in gamma-ray astronomy. The workshop will be organized in sessions dedicated to:
The soft gamma-ray sky:
Surveys
and observations from: INTEGRAL, SWIFT, SUZAKU, MAXI etc
The high energy gamma-ray sky:
Surveys
and observations from: AGILE, FERMI, HESS, MAGIC etc
The search for counterparts:
Synergies between surveys: The multi-waveband approach
Comparing and contrasting the two skies:
Similarities and differences: which theoretical implications, New
source typologies: what have we learnt
Prospects for
future missions above 10 keV: Decadal Survey, Cosmic Vision
national programmes etc.
Scientific Organizing Committee
F.
Aharonian
(DIAS/Dublin, Ireland and MPIK/Heidelberg Germany)
M. Ajello
(SLAC, Menlo
Park, USA)
A.J. Bird
(Southampton University, UK)
P.
Caraveo
(INAF/IASF-Milano, Ital)
A.
De Angelis
(Universita’ di Udine, Italy)
R.
Diehl
(MPE Garching, Germany)
N.
Gehrels
(NASA/GSFC, Greenbelt, USA),
I.
A. Grenier
(University of Paris Denis
Diderot/CEA Saclay,
France)
W. Hermsen
(SRON, Amsterdam, The Netherlands)
M. Matsuoka
(JAXA/ISAS, Tsukuba, Japan)
P. Michelson
(Standford University, USA)
J.P. Roques
(CESR, Toulouse, France)
J.B. Stephen
(INAF/IASF-Bologna, Italy, Co-Chair)
R.
Sunyaev
(MPI fuer Astrophysik, Germany)
M.
Tavani
(INAF/IASF-Roma,
Italy)
P. Ubertini
(INAF/IASF-Roma, Italy, Co-Chair)
C.
Winkler
(ESA/ESTEC, Noordwijk, The Netherlands)
Local
Organizing Committee
C. Spalletta
(INAF/IASF-Roma, Italy)
M. Del Santo
(INAF/IASF-Roma, Italy)
A. Malizia
(INAF/IASF-Bologna, Italy)
G. Sabatino
(INAF/IASF-Roma, Italy)
E. Scalise
(INAF/IASF-Roma, Italy)
INAF/IASF
- Via Fosso del
Cavaliere 100, 00133 Rome - Italy - tel + 39 06 49934090 - fax + 39 06
49934092 | ||||||||||||||||||||||||||||||||||||||||||||