Conveners
Plenary
- Jisuke Kubo (Kanazawa University)
Plenary
- Jun'ichi Yokoyama (The University of Tokyo)
Plenary
- Nicole Bell (University of Melbourne)
Plenary
- Gary Hill (University of Adelaide)
Plenary
- Christian Reichardt (University of Melbourne)
Plenary
- mihoko nojiri (KEK)
Plenary
- Antoine David Kouchner (Universite de Paris VII (FR))
Plenary
- Matthieu TRISTRAM (CNRS)
Plenary
- Csaba Balazs (Monash University)
Plenary
- Sang Pyo Kim (Kunsan National University)
Description of the Pierre Auger cosmic ray detector
Measurements of the energy spectrum, the arrival directions and the mass composition.
Searches for high energy photons, neutrons, neutrinos and high energy magnetic monopoles.
ARCA (Astroparticle Research with Cosmics in the Abyss) is the high-energy neutrino telescope being built as part of the KM3NeT deep-sea research infrastructure. Optimised for a high angular resolution to neutrinos in the TeV-PeV regime, its main physics goals are the exploration of the high-energy astrophysical neutrino signal reported by IceCube, and the discovery of Galactic neutrino...
The IceCube Neutrino Observatory is the world’s largest neutrino detector. Located at the South Pole, IceCube consists of a cubic kilometre of ice instrumented with 5160 photomultiplier tubes on 86 strings at a depth of 1.5-2.5 km. In this talk I will present the latest results concerning the high-energy neutrinos detected by IceCube. Plans for a next-generation IceCube detector, named...
The present epoch Universe is inhomogeneous on < 100/h Mpc scales, opening up the possibility of backreaction - that average cosmic expansion is significantly different from that of the standard FLRW geometry at late epochs. Realizing this possibility means confronting unsolved open questions in general relativity, in particular the nonlocal nature of gravitational energy in coarse-graining...
The Dark Energy Survey (DES) is in its fourth year of a five year observing program. We’re on our way to mapping 300 million galaxies and measuring 3000 type Ia supernovae for dark energy studies as well as monitoring 800 Active galaxies so we can use reverberation mapping to measure supermassive black hole masses across the last 12 billion years (to z~4). Over 525 nights DES combines a...
