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@article{Abe:2017:1538-4357/aa951b,
author = {Abe, K and Bronner, C and Pronost, G and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kato, Y and Kishimoto, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Okajima, Y and Orii, A and Sekiya, H and Shiozawa, M and Sonoda, Y and Takeda, A and Takenaka, A and Tanaka, H and Tasaka, S and Tomura, T and Akutsu, R and Kajita, T and Kaneyuki, K and Nishimura, Y and Okumura, K and Tsui, KM and Labarga, L and Fernandez, P and Blaszczyk, FDM and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Tobayama, S and Goldhaber, M and Elnimr, M and Kropp, WR and Mine, S and Locke, S and Weatherly, P and Smy, MB and Sobel, HW and Takhistov, V and Ganezer, KS and Hill, J and Kim, JY and Lim, IT and Park, RG and Himmel, A and Li, Z and O'Sullivan, E and Scholberg, K and Walter, CW and Ishizuka, T and Nakamura, T and Jang, JS and Choi, K and Learned, JG and Matsuno, S and Smith, SN and Amey, J and Lit},
doi = {1538-4357/aa951b},
journal = {Astrophysical Journal},
title = {Search for an Excess of Events in the Super-Kamiokande Detector in the Directions of the Astrophysical Neutrinos Reported by the IceCube Collaboration},
url = {http://dx.doi.org/10.3847/1538-4357/aa951b},
volume = {850},
year = {2017}
}

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TY  - JOUR
AB  - We present the results of a search in the Super-Kamiokande (SK) detector for excesses of neutrinos with energies above a few GeV that are in the direction of the track events reported in IceCube. Data from all SK phases (SK-I through SK-IV) were used, spanning a period from 1996 April to 2016 April and corresponding to an exposure of 225 kiloton-years. We considered the 14 IceCube track events from a data set with 1347 livetime days taken from 2010 to 2014. We use Poisson counting to determine if there is an excess of neutrinos detected in SK in a 10° search cone (5° for the highest energy data set) around the reconstructed direction of the IceCube event. No significant excess was found in any of the search directions we examined. We also looked for coincidences with a recently reported IceCube multiplet event. No events were detected within a ±500 s time window around the first detected event, and no significant excess was seen from that direction over the lifetime of SK.
AU  - Abe,K
AU  - Bronner,C
AU  - Pronost,G
AU  - Hayato,Y
AU  - Ikeda,M
AU  - Iyogi,K
AU  - Kameda,J
AU  - Kato,Y
AU  - Kishimoto,Y
AU  - Marti,L
AU  - Miura,M
AU  - Moriyama,S
AU  - Nakahata,M
AU  - Nakano,Y
AU  - Nakayama,S
AU  - Okajima,Y
AU  - Orii,A
AU  - Sekiya,H
AU  - Shiozawa,M
AU  - Sonoda,Y
AU  - Takeda,A
AU  - Takenaka,A
AU  - Tanaka,H
AU  - Tasaka,S
AU  - Tomura,T
AU  - Akutsu,R
AU  - Kajita,T
AU  - Kaneyuki,K
AU  - Nishimura,Y
AU  - Okumura,K
AU  - Tsui,KM
AU  - Labarga,L
AU  - Fernandez,P
AU  - Blaszczyk,FDM
AU  - Gustafson,J
AU  - Kachulis,C
AU  - Kearns,E
AU  - Raaf,JL
AU  - Stone,JL
AU  - Sulak,LR
AU  - Berkman,S
AU  - Tobayama,S
AU  - Goldhaber,M
AU  - Elnimr,M
AU  - Kropp,WR
AU  - Mine,S
AU  - Locke,S
AU  - Weatherly,P
AU  - Smy,MB
AU  - Sobel,HW
AU  - Takhistov,V
AU  - Ganezer,KS
AU  - Hill,J
AU  - Kim,JY
AU  - Lim,IT
AU  - Park,RG
AU  - Himmel,A
AU  - Li,Z
AU  - O'Sullivan,E
AU  - Scholberg,K
AU  - Walter,CW
AU  - Ishizuka,T
AU  - Nakamura,T
AU  - Jang,JS
AU  - Choi,K
AU  - Learned,JG
AU  - Matsuno,S
AU  - Smith,SN
AU  - Amey,J
AU  - Litchfield,RP
AU  - Ma,WY
AU  - Uchida,Y
AU  - Wascko,MO
AU  - Cao,S
AU  - Friend,M
AU  - Hasegawa,T
AU  - Ishida,T
AU  - Ishii,T
AU  - Kobayashi,T
AU  - Nakadaira,T
AU  - Nakamura,K
DO  - 1538-4357/aa951b
PY  - 2017///
SN  - 0004-637X
TI  - Search for an Excess of Events in the Super-Kamiokande Detector in the Directions of the Astrophysical Neutrinos Reported by the IceCube Collaboration
T2  - Astrophysical Journal
UR  - http://dx.doi.org/10.3847/1538-4357/aa951b
UR  - http://hdl.handle.net/10044/1/56047
VL  - 850
ER  -

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Morgan O. Wascko

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