908 citations · 4.3k across the 154 of their papers we have counts for
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Unveiling the substructure of the massive clump AGAL G035.133000.7450
M. E. Ortega, A. Marinelli, N. L. Isequilla +1
It is known that massive stars form as result of the fragmentation of molecular clumps. However, what is not clear is whether this fragmentation gives rise to cores massive enough…
Search for non-standard neutrino interactions with 10 years of ANTARES data
A. Albert, S. Alves, M. André +145
Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Ear…
Nanobeacon: A time calibration device for the KM3NeT neutrino telescope
S. Aiello, A. Albert, M. Alshamsi +238
The KM3NeT Collaboration is currently constructing a multi-site high-energy neutrino telescope in the Mediterranean Sea consisting of matrices of pressure-resistant glass spheres,…
KM3NeT/ARCA expectations in view of a novel multimessenger study of starburst galaxies
Antonio Marinelli, Antonio Ambrosone, Walid Idrissi Ibnsalih +4
Starburst galaxies (SBGs) and more in general starforming galaxies represent a class of galaxies with a high star formation rate (up to 100 solar masses/year). Despite their low lu…
Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources
Antonio Galván, Nissim Fraija, Edilberto Aguilar-Ruiz +3
The detection of the high-energy neutrino IC-170922A in spatial (within the error region) and temporal flare activity correlation with the blazar TXS 0506+056 allowed these objects…
Acoustic Neutrino Detection In a Adriatic Multidisciplinary Observatory (ANDIAMO)
Antonio Marinelli, Pasquale Migliozzi, Andreino Simonelli
The existence of cosmic accelerators able to emit charged particles up to EeV energies has been confirmed by the observations made in the last years by experiments such as Auger an…
Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search
KM3NeT Collaboration, S. Aiello, A. Albert +242
The KM3NeT research infrastructure is under construction in the Mediterranean Sea. KM3NeT will study atmospheric and astrophysical neutrinos with two multi-purpose neutrino detecto…
Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering
KM3NeT Collaboration, S. Aiello, A. Albert +275
This article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interes…
The Calibration Units of KM3NeT
R. Le Breton, M. Billault, C. Boutonnet +16
KM3NeT is a deep-sea infrastructure composed of two neutrino telescopes being deployed in the Mediterranean Sea: ARCA, near Sicily in Italy, designed for neutrino astronomy, and OR…
Cyano radical emission at small spatial scales towards massive protostars
S. Paron, M. E. Ortega, A. Marinelli +2
The cyano radical (CN), one of the first detected interstellar molecular species, is a key molecule in many astrochemical chains. Particularly, it is detected towards molecular cor…
Comparison of the measured atmospheric muon rate with Monte Carlo simulations and sensitivity study for detection of prompt atmospheric muons with KM3NeT
Piotr Kalaczyński
The KM3NeT Collaboration has successfully deployed the first detection units of the next generation undersea neutrino telescopes in the Mediterranean Sea at the two sites in Italy…
Studying Bioluminescence Flashes with the ANTARES Deep Sea Neutrino Telescope
N. Reeb, S. Hutschenreuter, P. Zehetner +141
We develop a novel technique to exploit the extensive data sets provided by underwater neutrino telescopes to gain information on bioluminescence in the deep sea. The passive natur…
Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
S. Aiello, A. Albert, M. Alshamsi +245
KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light steri…
Could nearby star-forming galaxies light up the point-like neutrino sky?
Antonio Ambrosone, Marco Chianese, Damiano F. G. Fiorillo +2
Star-forming and starburst galaxies, which are well-known cosmic-rays reservoirs, are expected to emit gamma-rays and neutrinos predominantly via hadronic collisions. In this Lette…
The KM3NeT potential for the next core-collapse supernova observation with neutrinos
KM3NeT Collaboration, S. Aiello, A. Albert +245
The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophys…
Search for neutrinos from the tidal disruption events AT2019dsg and AT2019fdr with the ANTARES telescope
ANTARES Collaboration, A. Albert, S. Alves +141
On October 1, 2019, the IceCube Collaboration detected a muon track neutrino with high probability of being of astrophysical origin, IC191001A. After a few hours, the tidal disrupt…
Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCA
S. Aiello, A. Albert, S. Alves Garre +239
The next generation of water Cherenkov neutrino telescopes in the Mediterranean Sea are under construction offshore France (KM3NeT/ORCA) and Sicily (KM3NeT/ARCA). The KM3NeT/ORCA d…