During the SN 1987A, the following gravitational wave (gw) and neutrino detectors were in operation:(a) the Maryland room-temperature gw antenna,(b) the Rome room-temperature gw antenna,(c) the Mont Blanc (LSD-UNO) neutrino detector,(d) the Kamiokande I1 neutrino detector,(e) the IMB neutrino detector, and (f) the Baksan neutrino detector.
Coincidences among the Maryland and Rome Gravitational Wave Detector Data and the Mont Blanc and Kamioka neutrino Detector Data in the Period of SN1987A
MG Castellano;
1989
Abstract
During the SN 1987A, the following gravitational wave (gw) and neutrino detectors were in operation:(a) the Maryland room-temperature gw antenna,(b) the Rome room-temperature gw antenna,(c) the Mont Blanc (LSD-UNO) neutrino detector,(d) the Kamiokande I1 neutrino detector,(e) the IMB neutrino detector, and (f) the Baksan neutrino detector.File in questo prodotto:
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