02/10/2018, 08:00
02/10/2018, 08:10
Ignacio Taboada
02/10/2018, 08:25
Anna Franckowiak
(DESY)
02/10/2018, 08:48
Chad Finley
(Stockholm University)
02/10/2018, 09:06
Prof.
Antoine Kouchner
(APC)
02/10/2018, 09:25
Anatoli Fedynitch
(DESY)
02/10/2018, 10:20
Michael Kachelriess
(NTNU)
02/10/2018, 10:50
Chad Finley
(Stockholm University)
02/10/2018, 11:20
Giulia Illuminati
(Instituto de Física Corpuscular)
02/10/2018, 13:30
Dr
Alexey Lubashevskiy
(JINR)
02/10/2018, 13:30
Dr
Evgeny Yakushev
(JINR)
02/10/2018, 13:50
Mr
Theo Glauch
(Technical University of Munich)
02/10/2018, 13:50
Alexandr Doroshenko
(INR RAS)
02/10/2018, 13:50
Christoph Raab
(ULB)
02/10/2018, 14:10
Lew Classen
(University of Muenster)
02/10/2018, 14:10
Juan Aguilar Sánchez
(Université Libre de Bruxelles (ULB))
02/10/2018, 14:15
Juliana Stachurska
(DESY Zeuthen)
02/10/2018, 14:30
Sara Rebecca Gozzini
(IFIC)
02/10/2018, 14:40
Konstantinos Pikounis
(NCSR Demokritos)
02/10/2018, 14:50
Prof.
Roumen Tsenov
(LHEP JINR)
02/10/2018, 15:05
Dr
Ronald Bruijn
(University of Amsterdam and Nikhef)
02/10/2018, 15:50
Prof.
Alexander Olshevskiy
(JINR)
02/10/2018, 15:50
Prof.
Donglian Xu
(Shanghai Jiao Tong University)
02/10/2018, 15:50
Ms
Lisa Schumacher
(RWTH Aachen)
02/10/2018, 16:08
Ms
Alba Domi
(Università degli Studi di Genova, INFN-Genova, CPPM-Marseille)
02/10/2018, 16:10
Mr
David Calvo
(IFIC)
02/10/2018, 16:10
Prof.
Aya Ishihara
(Chiba University)
02/10/2018, 16:26
Alexander Kappes
(University Muenster)
02/10/2018, 16:30
Dr
Joshua Hignight
(Dr.)
02/10/2018, 16:30
Yuya Makino
(Chiba University)
02/10/2018, 16:50
Dr
Dmitry Naumov
(JINR)
02/10/2018, 16:50
Mr
Christian Haack
(RWTH Aachen University)
02/10/2018, 17:02
Dr
Joshua Hignight
(Dr.)
02/10/2018, 17:10
Mr
Grigory Safronov
(JINR)
02/10/2018, 17:20
Viacheslav Egorov
(JINR)
02/10/2018, 17:20
Prof.
Dmitry Naumov
(DLNP JINR)
03/10/2018, 08:00
Elisa Püschel
03/10/2018, 08:20
Anna Franckowiak
(DESY)
03/10/2018, 08:50
Maxim Pshirkov
(Lomonosov Moscow State University, SAI)
03/10/2018, 09:20
Dr
Vladimir Aynutdinov
(INR RAS)
03/10/2018, 10:20
Paschal Coyle
(Centre de Physique des particules de Marseille)
03/10/2018, 10:45
Jürgen Brunner
(CPPM)
03/10/2018, 11:10
Prof.
Alexandre Zaitsev
(IHEP NRC KI)
03/10/2018, 11:35
Véronique Van Elewyck
(APC, Université Paris Diderot)
03/10/2018, 13:20
Prof.
Zhan-Arys Dzhilkibaev
(Institute for nuclear research)
03/10/2018, 13:20
Dr
Irene Di Palma
(University of Rome Sapienza and INFN)
03/10/2018, 13:20
Nikolai Budnev
(Irkutsk State University)
03/10/2018, 13:38
Mrs
Federica Bradascio
(DESY)
03/10/2018, 13:40
Mr
David Calvo
(IFIC)
03/10/2018, 13:40
Mr
Christian Haack
(RWTH Aachen University)
03/10/2018, 14:00
Antonino Capone
(Physics Department University “La Sapienza” and INFN, Roma, Italy)
03/10/2018, 14:19
Mr
Alexander Avrorin
(INR RAS)
03/10/2018, 14:20
Marta Colomer Molla
(APC/IFIC)
03/10/2018, 14:20
Dr
Dominique Lefevre
(CNRS MIO)
03/10/2018, 14:37
Alexander Shestyakov
03/10/2018, 14:40
Elisa Resconi
(TU Munich)
03/10/2018, 15:00
Pablo Marín Jímenez
03/10/2018, 15:00
Mr
James DeLaunay
(Penn State)
03/10/2018, 15:50
Dr
Tommaso Chiarusi
(INFN-Sezione di Bologna)
03/10/2018, 15:50
Anatoly Petrukhin
(MEPhI)
03/10/2018, 15:50
Dr
Ronald Bruijn
(University of Amsterdam and Nikhef)
03/10/2018, 16:10
Mr
Felix Henningsen
(TUM)
03/10/2018, 16:10
Dr
Ludwig Rauch
(DESY)
03/10/2018, 16:10
Bruny Baret
(APC-CNRS)
03/10/2018, 16:30
Evgeny Khramov
(JINR)
03/10/2018, 16:30
Dr
Cristiano Bozza
(University of Salerno and INFN Gruppo Collegato di Salerno)
03/10/2018, 16:30
Jannik Hofestaedt
(ECAP, Uni Erlangen-Nürnberg)
03/10/2018, 16:50
Anna Franckowiak
(DESY)
03/10/2018, 16:50
Dr
Tommaso Chiarusi
(INFN-Sezione di Bologna)
03/10/2018, 16:50
Prof.
Zhan-Arys Dzhilkibaev
(Institute for nuclear research)
03/10/2018, 17:10
Mr
Konstantinos Pikounis
(NCSR Demokritos)
03/10/2018, 17:10
Dr
Tim Ruhe
(TU Dortmund)
04/10/2018, 08:00
Dr
Leonid Kuzmichev
(SINP)
04/10/2018, 08:20
Dr
Chiara De Sio
(INFN)
04/10/2018, 08:25
Yuri Stenkin
(INR RAS)
04/10/2018, 08:40
Mirco Huennefeld
(TU Dortmund)
04/10/2018, 08:50
Dr
Tim Ruhe
(TU Dortmund)
04/10/2018, 09:00
Dr
Alexander Kryukov
(SINP MSU)
04/10/2018, 09:15
Dmitriy Kostunin
(Karlsruhe Institute of Technology (KIT))
04/10/2018, 09:20
Marek Kowalski
(DESY and Humboldt-University)
04/10/2018, 10:10
Alexander Kappes
(University Muenster)
04/10/2018, 10:30
Christian Spiering
04/10/2018, 10:45
Jannik Hofestädt
(ECAP, Uni Erlangen-Nürnberg)
04/10/2018, 11:00
Prof.
Uli Katz
(ECAP / Univ. Erlangen)
04/10/2018, 11:15
Juan Antonio Aguilar Sanchez
(Université Libre de Bruxelles (ULB))
The nature of dark matter remains one of the most enduring unsolved questions in modern cosmology. In order to decipher the mystery of dark matter and understand its properties different experimental avenues are explored. Indirect searches make use of the annihilation or decay products of dark matter as traces to prove its existence. This strategy is complementary of direct detection as...
Christoph Raab
(Université libre de Bruxelles)
Blazars have long been considered as accelerator candidates for cosmic rays. In such a scenario, hadronic interactions in their jet would produce neutrinos and gamma-rays. Correlating the astrophysical neutrinos detected by IceCube, a cubic-kilometre neutrino telescope at the South Pole, with the gamma-ray emission from blazars could therefore reveal the origin of cosmic rays. In our method we...
Mr
Christian Haack
(RWTH Aachen University)
Many neutrino interactions measured by the IceCube Neutrino Observatory produce only hadronic showers, which appear as almost point-like light emission due to the large detector spacing (~125m). At PeV energies these showers often saturate the PMTs closest to the interaction vertex - thus the reconstruction has to rely on more diffused photons which requires precise understanding of the...
Dr
Cristiano Bozza
(University of Salerno and INFN Gruppo Collegato di Salerno)
The multi-site nature of the KM3NeT collaboration has influenced the development and evolution of its Acquisition Control software. It is flexible and portable to the extent that the same programs are used in data-taking shore station of neutrino telescopes as well as in the test and qualification sites for performance and quality assessment of detector components at different stages of the...
Dr
Cristiano Bozza
(University of Salerno and INFN Gruppo Collegato di Salerno)
The multi-site nature of the KM3NeT project has influenced the development
and evolution of its acquisition control software so that it doesn’t stick to a
single detector site or configuration. It is flexible and portable to the extent that
the same programs are used in data-taking shore station of neutrino
telescopes as well as in testing sites for detector components at...
Ignacio Taboada
(Georgia Institute of Technology)
Cosmic rays and neutrinos are intimately related. And though TeV-PeV astrophysical neutrinos have been observed, their sources and their relation to potential sources of cosmic rays remain largely unknown. IceCube has conducted numerous searches for potential neutrino sources. This talk is an overview that complements other presentations at this conference.
I will describe the...
Elisa Pueschel
(Deutsches Elektronen-Synchrotron)
The very-high-energy gamma-ray sky grows ever more populated, with over 200 sources. The current-generation imaging atmospheric Cherenkov telescope arrays, VERITAS, H.E.S.S. and MAGIC, have collected over a decade of observations covering an energy range from tens of GeV to tens of TeV, while HAWC has collected several years of survey observations in the TeV to 100 TeV energy range. These...
Antoine Kouchner
(University Paris Diderot -- APC)
ANTARES, the largest underwater neutrino telescope, has been continuously operating since 2007 in the Mediterranean Sea. The transparency of the water allows for a very good angular resolution in the reconstruction of neutrino events of all flavors. This results in an unmatched sensitivity for neutrino source searches, in a large fraction of the Southern Sky at TeV energies. As a consequence,...
Roumen Tsenov
Ronald Bruijn
(University of Amsterdam and Nikhef)
The KM3NeT Collaboration is constructing new-generation neutrino detectors in the Mediterranean Sea. The main goals are the study of the high-energy neutrino flux (KM3NeT/ARCA, off-shore Capo-Passero, Italy) and the determination of the neutrino mass ordering (KM3NeT/ORCA, off-shore Toulon, France). The basic detection element, the Digital Optical Module (DOM), houses 31 three-inch PMT’s...