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27 April 2024
 
  » arxiv » 1703.9284

 Article overview



Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
B. Bartoli ; P. Bernardini ; X. J. Bi ; Z. Cao ; S. Catalanotti ; S. Z. Chen ; T. L. Chen ; S. W. Cui ; B. Z. Dai ; A. D Amone ; Danzeng Luobu ; I. De Mitri ; B. D Ettorre Piazzoli ; T. Di Girolamo ; G. Di Sciascio ; C. F. Feng ; Zhaoyang Feng ; Zhenyong Feng ; W. Gao ; Q. B. Gou ; Y. Q. Guo ; H. H. He ; Haibing Hu ; Hongbo Hu ; M. Iacovacci ; R. Iuppa ; H. Y. Jia ; Labaci Ren ; H. J. Li ; C. Liu ; J. Liu ; M. Y. Liu ; H. Lu ; L. L. Ma ; X. H. Ma ; G. Mancarella ; S. M. Mari ; G. Marsella ; S. Mastroianni ; P. Montini ; C. C. Ning ; L. Perrone ; P. Pistilli ; P. Salvini ; R. Santonico ; P. R. Shen ; X. D. Sheng ; F. Shi ; A. Surdo ; Y. H. Tan ; P. Vallania ; S. Vernetto ; C. Vigorito ; H. Wang ; C. Y. Wu ; H. R. Wu ; L. Xue ; Q. Y. Yang ; X. C. Yang ; Z. G. Yao ; A. F. Yuan ; M. Zha ; H. M. Zhang ; L. Zhang ; X. Y. Zhang ; Y. Zhang ; J. Zhao ; Zhaxici Ren ; Zhaxisang Zhu ; X. X. Zhou ; F. R. Zhu ; Q. Q. Zhu ;
Date 23 Mar 2017
AbstractThe 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.
Source arXiv, 1703.9284
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