| Published Articles | |
| Report number | arXiv:1703.09284 |
| Title | Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode |
| Related title | Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode |
| Author(s) |
Bartoli, B. (INFN, Naples ; Naples U.) ; Bernardini, P. (INFN, Lecce ; Salento U.) ; Bi, X.J. (Beijing, Inst. High Energy Phys.) ; Cao, Z. (Beijing, Inst. High Energy Phys.) ; Catalanotti, S. (INFN, Naples ; Naples U.) ; Chen, S.Z. ; Chen, T.L. (Tibet U.) ; Cui, S.W. (Hebei Normal U.) ; Dai, B.Z. (Yunnan U.) ; D'Amone, A. (Salento U. ; INFN, Lecce) ; Danzengluobu (Tibet U.) ; De Mitri, I. (INFN, Lecce ; Salento U.) ; Ettorre Piazzoli, B.D. (Turin U.) ; Girolamo, T.Di (Naples U. ; INFN, Naples) ; Di Sciascio, G. (INFN, Rome2) ; Feng, C.F. (Shandong U.) ; Feng, Zhaoyang (Beijing, Inst. High Energy Phys.) ; Feng, Zhenyong (Southwest Jiaotong U.) ; Gao, W. (CERN) ; Gou, Q.B. (Beijing, Inst. High Energy Phys.) ; Guo, Y.Q. (Beijing, Inst. High Energy Phys.) ; He, H.H. (Beijing, Inst. High Energy Phys.) ; Hu, Haibing (Tibet U.) ; Hu, Hongbo (Beijing, Inst. High Energy Phys.) ; Iacovacci, M. (INFN, Naples ; Naples U.) ; Iuppa, R. (TIFPA-INFN, Trento ; Trento U.) ; Jia, H.Y. (Southwest Jiaotong U.) ; Labaciren (Tibet U.) ; Li, H.J. (Tibet U.) ; Liu, C. (Southern Methodist U.) ; Liu, J. (Western Australia U.) ; Liu, M.Y. (Tibet U.) ; Lu, H. (Huangshan U.) ; Ma, L.L. (Shandong U.) ; Ma, X.H. (Beijing, Inst. High Energy Phys.) ; Mancarella, G. (INFN, Lecce ; Salento U.) ; Mari, S.M. (INFN, Rome) ; Marsella, G. (INFN, Lecce ; Salento U.) ; Mastroianni, S. (INFN, Naples) ; Montini, P. (INFN, Rome2) ; Ning, C.C. (Tibet U.) ; Perrone, L. (INFN, Lecce ; Salento U.) ; Pistilli, P. (INFN, Rome3 ; Rome III U.) ; Salvini, P. (INFN, Pavia) ; Santonico, R. (INFN, Rome ; Rome U., Tor Vergata) ; Shen, P.R. (Beijing, Inst. High Energy Phys.) ; Sheng, X.D. (Beijing, Inst. High Energy Phys.) ; Shi, F. (Beijing, Inst. High Energy Phys.) ; Surdo, A. (INFN, Lecce) ; Tan, Y.H. (Beijing, Inst. High Energy Phys.) ; Vallania, P. (INFN, Turin ; Turin Observ.) ; Vernetto, S. (INFN, Turin ; Turin Observ.) ; Vigorito, C. (INFN, Turin ; Turin U.) ; Wang, H. (UCLA) ; Wu, C.Y. (Beijing, Inst. High Energy Phys.) ; Wu, H.R. (Beijing, Inst. High Energy Phys.) ; Xue, L. (Shandong U.) ; Yang, Q.Y. (Yunnan U.) ; Yang, X.C. (Yunnan U.) ; Yao, Z.G. (Beijing, Inst. High Energy Phys.) ; Yuan, A.F. (Tibet U.) ; Zha, M. (Beijing, Inst. High Energy Phys.) ; Zhang, H.M. (Beijing, Inst. High Energy Phys.) ; Zhang, L. (Tsinghua U., Beijing) ; Zhang, X.Y. (Shandong U.) ; Zhang, Y. (Columbia U.) ; Zhao, J. (Purdue U.) ; Zhaxiciren (Tibet U.) ; Zhaxisangzhu (Tibet U.) ; Zhou, X.X. (Lanzhou, Inst. Modern Phys.) ; Zhu, F.R. (Southwest Jiaotong U.) ; Zhu, Q.Q. (Beijing, Inst. High Energy Phys.) |
| Publication | 2017-06-09 |
| Imprint | 2017-03-23 |
| Number of pages | 11 |
| Note | 24pages and 12 figures |
| In: | Astrophys. J. |
| DOI | 10.3847/1538-4357/aa74bc 10.3847/1538-4357/aa74bc |
| Subject category | hep-ph ; Particle Physics - Phenomenology ; astro-ph.HE ; Astrophysics and Astronomy |
| Abstract | The ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a full coverage air shower array dedicated to gamma ray astronomy and cosmic ray studies. The wide field of view ( 2 sr) and high duty cycle (> 86%), made ARGO-YBJ suitable to search for short and unexpected gamma ray emissions like gamma ray bursts (GRBs). Between 2007 November 6 and 2013 February 7, 156 satellite-triggered GRBs (24 of them with known redshift) occurred within the ARGO-YBJ field of view. A search for possible emission associated to these GRBs has been made in the two energy ranges 10-100 GeV and 10-1000 GeV. No significant excess has been found in time coincidence with the satellite detections nor in a time window of one hour after the bursts. Taking into account the EBL absorption, upper limits to the energy fluence at 99% of confidence level have been evaluated,with values ranging from 10-5 erg cm-2 to 10-1 erg cm-2. |
| Copyright/License | CC-BY-NC-SA-4.0 |
Corresponding record in: Inspire
Zapis kreiran 2017-04-22, zadnja izmjena 2024-12-05
