Observation of multi-Tev gamma rays from MGRO J2019+37 and MGRO J2031+41 with the tibet air shower array

(The Tibet ASγ Collaboration)

Observation of multi-Tev gamma rays from MGRO J2019+37 and MGRO J2031+41 with the tibet air shower array

(The Tibet ASγ Collaboration)

Waseda Research Institute for Science and Engineering

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

The Tibet III air shower array is located at 4300 m above sea level, Tibet, China. Multi-TeV gamma rays were observed from MGRO J2019+37 and MGRO J2031+41 in the Cygnus region using data taken by the Tibet III air shower array in the period between 1999 and 2010.

Original language	English
Title of host publication	Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
Publisher	Sociedade Brasileira de Fisica
Volume	2013-October
ISBN (Electronic)	9788589064293
Publication status	Published - 2013 Jan 1
Event	33rd International Cosmic Rays Conference, ICRC 2013 - Rio de Janeiro, Brazil Duration: 2013 Jul 2 → 2013 Jul 9

Other

Other	33rd International Cosmic Rays Conference, ICRC 2013
Country/Territory	Brazil
City	Rio de Janeiro
Period	13/7/2 → 13/7/9

Keywords

Cygnus region
Gamma rays
Tibet air shower array

ASJC Scopus subject areas

Nuclear and High Energy Physics

Cite this

@inproceedings{a3b49d71e3fa4e7a87a59efdab6d61ac,

title = "Observation of multi-Tev gamma rays from MGRO J2019+37 and MGRO J2031+41 with the tibet air shower array",

abstract = "The Tibet III air shower array is located at 4300 m above sea level, Tibet, China. Multi-TeV gamma rays were observed from MGRO J2019+37 and MGRO J2031+41 in the Cygnus region using data taken by the Tibet III air shower array in the period between 1999 and 2010.",

keywords = "Cygnus region, Gamma rays, Tibet air shower array",

author = "{(The Tibet ASγ Collaboration)} and M. Amenomori and Bi, {X. J.} and D. Chen and Chen, {T. L.} and Chen, {W. Y.} and Cui, {S. W.} and Danzengluobu and Ding, {L. K.} and Feng, {C. F.} and Zhaoyang Feng and Feng, {Z. Y.} and Gou, {Q. B.} and Guo, {Y. Q.} and He, {H. H.} and He, {Z. T.} and K. Hibino and N. Hotta and Haibing Hu and Hu, {H. B.} and J. Huang and Jia, {H. Y.} and L. Jiang and F. Kajino and K. Kasahara and Y. Katayose and C. Kato and K. Kawata and M. Kozai and Labaciren and Le, {G. M.} and Li, {A. F.} and Li, {H. J.} and Li, {W. J.} and C. Liu and Liu, {J. S.} and Liu, {M. Y.} and H. Lu and Meng, {X. R.} and K. Mizutani and K. Munakata and H. Nanjo and M. Nishizawa and M. Ohnishi and I. Ohta and Shunsuke Ozawa and Qian, {X. L.} and Qu, {X. B.} and T. Saito and Saito, {T. Y.} and Shoji Torii",

year = "2013",

month = jan,

day = "1",

language = "English",

volume = "2013-October",

booktitle = "Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013",

publisher = "Sociedade Brasileira de Fisica",

address = "Brazil",

note = "33rd International Cosmic Rays Conference, ICRC 2013 ; Conference date: 02-07-2013 Through 09-07-2013",

}

TY - GEN

T1 - Observation of multi-Tev gamma rays from MGRO J2019+37 and MGRO J2031+41 with the tibet air shower array

AU - (The Tibet ASγ Collaboration)

AU - Amenomori, M.

AU - Bi, X. J.

AU - Chen, D.

AU - Chen, T. L.

AU - Chen, W. Y.

AU - Cui, S. W.

AU - Danzengluobu,

AU - Ding, L. K.

AU - Feng, C. F.

AU - Feng, Zhaoyang

AU - Feng, Z. Y.

AU - Gou, Q. B.

AU - Guo, Y. Q.

AU - He, H. H.

AU - He, Z. T.

AU - Hibino, K.

AU - Hotta, N.

AU - Hu, Haibing

AU - Hu, H. B.

AU - Huang, J.

AU - Jia, H. Y.

AU - Jiang, L.

AU - Kajino, F.

AU - Kasahara, K.

AU - Katayose, Y.

AU - Kato, C.

AU - Kawata, K.

AU - Kozai, M.

AU - Labaciren,

AU - Le, G. M.

AU - Li, A. F.

AU - Li, H. J.

AU - Li, W. J.

AU - Liu, C.

AU - Liu, J. S.

AU - Liu, M. Y.

AU - Lu, H.

AU - Meng, X. R.

AU - Mizutani, K.

AU - Munakata, K.

AU - Nanjo, H.

AU - Nishizawa, M.

AU - Ohnishi, M.

AU - Ohta, I.

AU - Ozawa, Shunsuke

AU - Qian, X. L.

AU - Qu, X. B.

AU - Saito, T.

AU - Saito, T. Y.

AU - Torii, Shoji

PY - 2013/1/1

Y1 - 2013/1/1

N2 - The Tibet III air shower array is located at 4300 m above sea level, Tibet, China. Multi-TeV gamma rays were observed from MGRO J2019+37 and MGRO J2031+41 in the Cygnus region using data taken by the Tibet III air shower array in the period between 1999 and 2010.

AB - The Tibet III air shower array is located at 4300 m above sea level, Tibet, China. Multi-TeV gamma rays were observed from MGRO J2019+37 and MGRO J2031+41 in the Cygnus region using data taken by the Tibet III air shower array in the period between 1999 and 2010.

KW - Cygnus region

KW - Gamma rays

KW - Tibet air shower array

UR - http://www.scopus.com/inward/record.url?scp=85052368829&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85052368829&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:85052368829

VL - 2013-October

BT - Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013

PB - Sociedade Brasileira de Fisica

T2 - 33rd International Cosmic Rays Conference, ICRC 2013

Y2 - 2 July 2013 through 9 July 2013

ER -

Observation of multi-Tev gamma rays from MGRO J2019+37 and MGRO J2031+41 with the tibet air shower array

Abstract

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Keywords

ASJC Scopus subject areas

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