746 citations · 1.6k across the 9 of their papers we have counts for
8 papers · 1 filter
Measurement of charm production in neutrino charged-current interactions
A. Kayis-Topaksu, G. Önengüt, R. van Dantzig +85
The nuclear emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy from 1994 to 1997. In total about 10…
Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande
Kamiokande Collaboration, S. Desai, Y. Ashie +133
We present the results of indirect searches for Weakly Interacting Massive Particles (WIMPs) with 1679.6 live days of data from the Super-Kamiokande detector using neutrino-induced…
A search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I
J. Yoo
A search for periodic modulations of the solar neutrino flux was performed using the Super-Kamiokande-I data taken from May 31st, 1996 to July 15th, 2001. The detector's capability…
Search for anti-electron-neutrinos from the Sun at Super-Kamiokande-I
Kamiokande collaboration, Y. Gando
We present the results of a search for low energy from the Sun using 1496 days of data from Super-Kamiokande-I. We observe no significant excess of events and set an uppe…
Search for Supernova Relic Neutrinos at Super-Kamiokande
Kamiokande Collaboration
A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-…
Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data
Kamiokande Collaboration
A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two all…
Super-Kamiokande atmospheric neutrino results
Toshiyuki Toshito, the Super-Kamiokande collaboration
We present atmospheric neutrino results from a 79 kiloton year (1289 days) exposure of the Super-Kamiokande detector. Our data are well explained by 2-flavor oscillat…
16-N as a calibration source for Super-Kamiokande
Kamiokande Collaboration, E. Blaufuss, G. Guillian
The decay of 16-N is used to cross check the absolute energy scale calibration for solar neutrinos established by the electron linear accelerator (LINAC). A deuterium-tritium neutr…