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Bartoli, B; Bernardini, P; Bi, X J; Bleve, C; Bolognino, I; Branchini, P; Budano, A; Calabrese Melcarne, A K; Camarri, P; Cao, Z; Cardarelli, R; Catalanotti, S; Cattaneo, C; Chen, S Z; Chen, T L; Chen, Y; Creti, P; Cui, S W; Dai, B Z; Staiti, G D'Alí; Danzengluobu; Dattoli, M; De Mitri, I; B D'Ettorre Piazzoli; T Di Girolamo; Ding, X H; G Di Sciascio; Feng, C F; Feng, Zhaoyang; Feng, Zhenyong; Galeazzi, F; Giroletti, E; Gou, Q B; Guo, Y Q; He, H H; Hu, Haibing; Hu, Hongbo; Huang, Q; Iacovacci, M; Iuppa, R; James, I; Jia, H Y; Labaciren; Li, H J; Li, J Y; Liguori, G; Liu, C; Liu, C Q; Liu, M Y; H Lu; Ma, L L; Ma, X H; Mancarella, G; Mari, S M; Marsella, G; Martello, D; Mastroianni, S; Montini, P; Ning, C C; Pagliaro, A; Panareo, M; Panico, B; Perrone, L; Pistilli, P; Ruggieri, F; Salvini, P; Shen, P R; Sheng, X D; Shi, F; Stanescu, C; Surdo, A; Tan, Y H; Vallania, P; Vernetto, S; Vigorito, C; Wang, B; Wang, H; Wu, C Y; Wu, H R; B Xu; Xue, L; Yang, Q Y; Yang, X C; Yao, Z G; Yuan, A F; Zha, M; Zhang, H M; Zhang, Jilong; Zhang, Jianli; Zhang, L; Zhang, P; Zhang, X Y; Zhang, Y; Zhao, J; Zhaxiciren; Zhaxisangzhu; Zhou, X X; Zhu, F R; Zhu, Q Q; Zizzi, G
arXiv.org, 01/2012Paper, Journal Article
We report the observation of TeV gamma-rays from the Cygnus region using the ARGO-YBJ data collected from 2007 November to 2011 August. Several TeV sources are located in this region including the two bright extended MGRO J2019+37 and MGRO J2031+41. According to the Milagro data set, at 20 TeV MGRO J2019+37 is the most significant source apart from the Crab Nebula. No signal from MGRO J2019+37 is detected by the ARGO-YBJ experiment, and the derived flux upper limits at 90% confidence level for all the events above 600 GeV with medium energy of 3 TeV are lower than the Milagro flux, implying that the source might be variable and hard to be identified as a pulsar wind nebula. The only statistically significant (6.4 standard deviations) gamma-ray signal is found from MGRO J2031+41, with a flux consistent with the measurement by Milagro.
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