| • • • We do not use the following data for averages, fits, limits, etc. • • • |
| $0.658$ $\pm0.016$ $\pm0.035$ |
1 |
|
SKAM |
| $0.702$ ${}^{+0.032}_{-0.030}$ $\pm0.101$ |
2 |
|
SKAM |
| $0.69$ $\pm0.10$ $\pm0.06$ |
3 |
|
SOU2 |
|
4 |
|
KAMI |
| $1.00$ $\pm0.15$ $\pm0.08$ |
5 |
|
FREJ |
| $0.60$ ${}^{+0.06}_{-0.05}$ $\pm0.05$ |
6 |
|
KAMI |
| $0.57$ ${}^{+0.08}_{-0.07}$ $\pm0.07$ |
7 |
|
KAMI |
|
8 |
|
IMB |
|
1
ASHIE 2005 results are based on an exposure of 92 kton yr during the complete Super-Kamiokande I running period. The analyzed data sample consists of fully-contained single-ring ${{\mathit e}}$-like events with 0.1 GeV/c $<{{\mathit p}_{{e}}}$ and ${{\mathit \mu}}$-like events 0.2 GeV/c $<{{\mathit p}_{{\mu}}}$, both having a visible energy $<$ 1.33 GeV. These criteria match the definition used by FUKUDA 1994 .
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2
ASHIE 2005 results are based on an exposure of 92 kton yr during the complete Super-Kamiokande I running period. The analyzed data sample consists of fully-contained single-ring events with visible energy $>$ 1.33 GeV and partially-contained events. All partially-contained events are classified as ${{\mathit \mu}}$-like.
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3
SANCHEZ 2003 result is based on an exposure of 5.9 kton yr, and updates ALLISON 1999 result. The analyzed data sample consists of fully-contained ${{\mathit e}}$-flavor and ${{\mathit \mu}}$-flavor events having lepton momentum $>$ 0.3 GeV/c.
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4
FUKUDA 1996B studied neutron background in the atmospheric neutrino sample observed in the Kamiokande detector. No evidence for the background contamination was found.
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5
DAUM 1995 results are based on an exposure of $2.0$ kton$~$yr which includes the data used by BERGER 1990B. This ratio is for the contained and semicontained events. DAUM 1995 also report $\mathit R({{\mathit \mu}}/{{\mathit e}}$) = $0.99$ $\pm0.13$ $\pm0.08$ for the total neutrino induced data sample which includes upward going stopping muons and horizontal muons in addition to the contained and semicontained events.
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6
FUKUDA 1994 result is based on an exposure of $7.7$ kton$~$yr and updates the HIRATA 1992 result. The analyzed data sample consists of fully-contained ${{\mathit e}}$-like events with $0.1<{{\mathit p}_{{e}}}<1.33$ GeV/$\mathit c$ and fully-contained ${{\mathit \mu}}$-like events with $0.2<{{\mathit p}_{{\mu}}}<1.5$ GeV/$\mathit c$.
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7
FUKUDA 1994 analyzed the data sample consisting of fully contained events with visible energy $>1.33$ GeV and partially contained ${{\mathit \mu}}$-like events.
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8
BECKER-SZENDY 1992B reports the fraction of nonshowering events (mostly muons from atmospheric neutrinos) as $0.36$ $\pm0.02$ $\pm0.02$, as compared with expected fraction $0.51$ $\pm0.01$ $\pm0.05$. After cutting the energy range to the Kamiokande limits, BEIER 1992 finds $\mathit R({{\mathit \mu}}/{{\mathit e}}$) very close to the Kamiokande value.
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