150 citations · 175 across the 6 of their papers we have counts for
7 papers
The Twisted Hilbert Space Ideals
Félix Cabello Sánchez, Ricardo García
We study those operators on a Hilbert space that can be lifted / extended to any twisted Hilbert space. We prove that these form an ideal of operators which contains all the Schatt…
Measurement of the neutron flux at the Canfranc Underground Laboratory with HENSA
S. E. A. Orrigo, J. L. Tain, N. Mont-Geli +14
We have performed a long-term measurement of the neutron flux with the High Efficiency Neutron Spectrometry Array HENSA in the Hall A of the Canfranc Underground Laboratory. The Ha…
First results from the HENSA/ANAIS collaboration at the Canfranc Underground Laboratory
N Mont-Geli, A Tarifeño-Saldivia, S E A Orrigo +24
The HENSA/ANAIS collaboration aims for the precise determination of the neutron flux that could affect ANAIS-112, an experiment looking for the dark matter annual modulation using…
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…
ANTARES upper limits on the multi-TeV neutrino emission from the GRBs detected by IACTs
ANTARES Collaboration, A. Albert, M. André +135
The first gamma-ray burst detections by Imaging Atmospheric Cherenkov Telescopes have been recently announced: GRB 190114C, detected by MAGIC, GRB 180720B and GRB 190829A, observed…
Using UV-pass filters for bright Moon observations with MAGIC
D. Guberman, J. Cortina, R. García +5
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes (IACT) that observe Very High Energy (VHE) gamma ray sources. The PMTs in their cameras are designed to operate un…
Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory
The Pierre Auger Collaboration, J. Abraham, P. Abreu +458
From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (a…