Dr
Shan Gao
(DESY)
12/10/16, 9:05 AM
AMON Workshop
Oral
Gamma-ray bursts (GRB) and blazars are luminous point sources in gamma-rays and candidate sources for IceCube neutrinos. The potential spatial and temporal correlations between
the IceCube neutrinos and the gamma-ray flares from those sources have called attention and extensive studies. Due to the low statistics of neutrino events, it is important to interpret the results based on accurate...
Dr
Robert Lauer
(University of New Mexico)
12/10/16, 11:10 AM
Dr
Daniela Dorner
(Universität Würzburg)
12/10/16, 11:30 AM
Dr
Fabian Schüssler
(IRFU / CEA-Saclay)
12/10/16, 11:50 AM
AMON Workshop
Oral
In this contribution I will present the H.E.S.S. programs to follow up on multi-wavelength and multi-messenger observations and alerts.
I will show first results from searches for high-energy gamma-ray emission in spatial coincidence with neutrino events detected by the IceCube and ANTARES neutrino telescopes and discuss recent extensions towards a fully integrated real-time alert system...
Dr
Chris Copperwheat
(Astrophysics Research Institute, Liverpool John Moores University)
12/10/16, 2:00 PM
AMON Workshop
Oral
The Liverpool Telescope is a 2-metre clear aperture, fully robotic telescope based at the Observatorio Del Roque De Los Muchachos on the Canary island of La Palma. Robotic telescopes are powerful tools for the exploration of the time variable sky, and their rapid reaction and flexible scheduling capabilities provide them with an important role in the multimessenger era. In this talk I will...
Prof.
Vladimir Lipunov
(Lomonosov Moscow State University)
12/10/16, 2:20 PM
Dr
Felicia Krauss
(GRAPPA & API, UvA)
12/10/16, 3:30 PM
AMON Workshop
Oral
The IceCube Collaboration has published results on a neutrino flux significantly in excess of the atmospheric background. Due to low atmospheric background at PeV energies, the highest energy events are the most likely ones to be of extraterrestrial origin. We use broadband spectra in the IceCube integration period to calculate the maximum expected number of neutrinos assuming a pion...