Detection of multi-TeV gamma rays from Markarian 501 during an unforeseen flaring state in 1997 with the Tibet air shower array

被引:41
作者
Amenomori, M [1 ]
Ayabe, S
Cao, PY
Danzengluobu
Ding, LK
Feng, ZY
Fu, Y
Guo, HW
He, M
Hibino, K
Hotta, N
Huang, Q
Huo, AX
Izu, K
Jia, HY
Kajino, F
Kasahara, K
Katayose, Y
Labaciren
Li, JY
Lu, H
Lu, SL
Luo, GX
Meng, XR
Mizutani, K
Mu, J
Nanjo, H
Nishizawa, M
Ohnishi, M
Ohta, I
Ouchi, T
Ren, JR
Saito, T
Sakata, M
Sasaki, T
Shi, ZZ
Shibata, M
Shiomi, A
Shirai, T
Sugimoto, H
Taira, K
Tan, YH
Tateyama, N
Torii, S
Utsugi, T
Wang, CR
Wang, H
Xu, XW
Yamamoto, Y
Yu, GC
机构
[1] Hirosaki Univ, Dept Phys, Hirosaki, Aomori 0368561, Japan
[2] Saitama Univ, Dept Phys, Urawa, Saitama 3388570, Japan
[3] Shandong Univ, Dept Phys, Jinan 250100, Peoples R China
[4] Tibet Univ, Dept Math & Phys, Lhasa 850000, Peoples R China
[5] Acad Sinica, Inst High Energy Phys, Beijing 100039, Peoples R China
[6] SW Jiaotong Univ, Dept Phys, Chengdu 610031, Peoples R China
[7] Kanagawa Univ, Fac Engn, Yokohama, Kanagawa 2218686, Japan
[8] Utsunomiya Univ, Fac Educ, Utsunomiya, Tochigi 3218505, Japan
[9] Univ Tokyo, Inst Cosm Ray Res, Tanashi, Tokyo 1888502, Japan
[10] Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan
[11] Shibaura Inst Technol, Fac Syst Engn, Omiya, Saitama 3308570, Japan
[12] Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China
[13] Natl Ctr Sci Informat Syst, Tokyo 1128640, Japan
[14] Tokyo Metropolitan Coll Aeronaut Engn, Tokyo 1160003, Japan
[15] Yokohama Natl Univ, Fac Engn, Yokohama, Kanagawa 2400067, Japan
[16] Shonan Inst Technol, Fujisawa, Kanagawa 2518511, Japan
关键词
BL Lacertae objects : individual (Markarian 501); gamma rays : observations;
D O I
10.1086/308558
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In 1997, the BL Lac object Mrk 501 entered a very active phase and was the brightest source in the sky at TeV energies, showing strong and frequent baring. Using the data obtained with a high-density air shower array that has been operating successfully at Yangbajing in Tibet since 1996, we searched for gamma-ray signals from this source during the period in 1997 from February through August. Our observation detected multi-TeV gamma-ray signals at the 3.7 sigma level during this period. The most rapid increase in the excess counts was observed between April 7 and June 16, and the statistical significance of the excess counts in this period was 4.7 sigma. Among several observations of flaring TeV gamma-rays from Mrk 501 in 1997, this is the only observation using a conventional air shower array. We present the energy spectrum of gamma-rays, which will be worth comparing with those obtained by imaging atmospheric Cerenkov telescopes.
引用
收藏
页码:302 / 307
页数:6
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