par Tiniakov, Petr 
;Okuda, Takeshi;Rubtsov, Grigory;Sagawa, Hiroyuki;Sakurai, Nobuyuki;Stokes, Benjamin B.T.;Takeda, Masahiro;Takeishi, R.;Taketa, Akimichi;Thomson, Gordon;Tkachev, Igor;Fukushima, Masaki;Tokuno, Hisao;Troitsky, Sergey ;Ikeda, Daisuke;Ivanov, Dmitry;Kawata, Kenji;Kido, Eiji;Matthews, John J.N.;Nagataki, Shigehiro;Nonaka, Toshiyuki
Référence Pos proceedings of science, 30-July-2015, 326
Publication Publié, 2015
;Okuda, Takeshi;Rubtsov, Grigory;Sagawa, Hiroyuki;Sakurai, Nobuyuki;Stokes, Benjamin B.T.;Takeda, Masahiro;Takeishi, R.;Taketa, Akimichi;Thomson, Gordon;Tkachev, Igor;Fukushima, Masaki;Tokuno, Hisao;Troitsky, Sergey ;Ikeda, Daisuke;Ivanov, Dmitry;Kawata, Kenji;Kido, Eiji;Matthews, John J.N.;Nagataki, Shigehiro;Nonaka, ToshiyukiRéférence Pos proceedings of science, 30-July-2015, 326
Publication Publié, 2015
Article révisé par les pairs
| Résumé : | The Telescope Array has collected 7 years of data. We make use of these data to search for large- and small-scale anisotropy of UHECR. At small angular scales we examine the data for clustering of events and correlations with some classes of putative sources. At large angular scales we present an update of the search for localized excesses by the oversampling method previously performed with the 5-year data set [1], and examine the data for correlations with the LSS of the Universe. We confirm the existence of the 'hot spot' of the radius 20 in the direction R:A: = 148:4, Dec: = 44:5 (equatorial coordinates) in the high-energy subset with E < 57 EeV. The post-trial significance of the hot spot in the 7-year data set is 3:4s, the same as in the 5-year data set. |
