Mobility Entropy and Message Routing in Community-Structured Delay Tolerant Networks Hideya Ochiai Hiroshi Esaki The University of Tokyo / NICT Asia Future.
Grand unification of AGN activity across the universe Nikos Fanidakis and C.M. Baugh, R.G. Bower, S. Cole, C. Done, C. S. Frenk 9 th Hellenic Astronomical.
SWNMediaKit2015
Identification of high energy gamma-ray sources and source populations in the era of deep all-sky coverage Olaf Reimer Stanford University Diego F. Torres.
The Multiwavelength Approach to Unidentified Gamma-Ray Sources MOTIVATION: Gamma-ray sources should be multiwavelength objects. X-RAYS:Counterpart searches.
1 Radio and Medium Access Control 2 Radio Properties.
ESTEC 7 Dec 2007 1 Radio Properties of the Moon: a brief review of some important bits Graham Woan University of Glasgow.
Joint formation and evolution of SMBHs and their host galaxies: How do the Quasar-Spheroid correlations change with the Cosmic Time? A. Treves Università.
Identification of high energy gamma-ray sources and source populations
What we (don’t) know about UHECRs We know: their energies (up to 10 20 eV). their overall energy spectrum We don’t know: where they are produced how.
Grand unification of AGN activity across the universe
