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The prototype detection unit of the KM3NeT detector
KM3NeT Collaboration, S. Adrián-Martínez, M. Ageron +246
A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80km offshore the Italian coast. KM3NeT in its final configuration will conta…
The On-Site Analysis of the Cherenkov Telescope Array
Andrea Bulgarelli, Valentina Fioretti, Andrea Zoli +54
The Cherenkov Telescope Array (CTA) observatory will be one of the largest ground-based very high-energy gamma-ray observatories. The On-Site Analysis will be the first CTA scienti…
Cherenkov Telescope Array Data Management
G. Lamanna, L. A. Antonelli, J. L. Contreras +37
Very High Energy gamma-ray astronomy with the Cherenkov Telescope Array (CTA) is evolving towards the model of a public observatory. Handling, processing and archiving the large am…
Optical and X-ray early follow-up of ANTARES neutrino alerts
S. Adrian-Martinez, M. Ageron, A. Albert +137
High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. Even with the recent detection of extr…
Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
S. Adrián-Martínez, A. Albert, M. André +127
The ANTARES experiment consists of an array of photomultipliers distributed along 12 lines and located deep underwater in the Mediterranean Sea. It searches for astrophysical neutr…
Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope
S. Adrián-Martínez, A. Albert, M. André +123
The ANTARES telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. The…