1.8k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of CataniaIT433 papers
- Centre National de la Recherche ScientifiqueFR334 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR297 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CataniaIT243 papers
- Istituto Nazionale di Fisica NucleareIT224 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT203 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT186 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR177 papers
- Sapienza University of RomeIT176 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT173 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT169 papers
- University of GenoaIT168 papers
4 papers · 2 filters
Optimizing the potential of KM3NeT in detecting core-collapse supernovae
KM3NeT Collaboration, O. Adriani, A. Albert +285
Core-collapse supernovae mark the end of life of massive stars. However, despite their importance in astrophysics, their underlying mechanisms remain unclear. Neutrinos that emerge…
Physical properties of long-rising type II supernovae -- Bayesian analytic modeling and spectrophotometric correlations
S. P. Cosentino, C. Inserra, M. L. Pumo
Supernova (SN) 1987A, with its long-rising (40 days) light curve, defines a rare subclass of type II SNe known as 1987A-like events. Representing only 1-3 percent of all c…
Explodability matters: how realistic neutrino-driven explosions change explosive nucleosynthesis yields
Luca Boccioli, Lorenzo Roberti
Explosive nucleosynthesis is affected by many uncertainties, particularly regarding assumptions and prescriptions adopted during the evolution of the star. Moreover, simple explosi…
Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A
KM3NeT Collaboration, O. Adriani, A. Albert +278
Context: The detection of the highest energy neutrino observed to date by KM3NeT, with an estimated energy of 220 PeV, opens up new possibilities for the study and identification o…