Search for GeV Gamma Ray Bursts with the ARGO-YBJ Detector: Summary of Eight Years of Observations
B. Bartoli, P. Bernardini, X.J. Bi, P. Branchini, A. Budano, P., Camarri, Z. Cao, R. Cardarelli, S. Catalanotti, S.Z. Chen, T.L. Chen, P., Creti, S.W. Cui, B.Z. Dai, A. D'Amone, Danzengluobu, I. De Mitri, B., D'Ettorre Piazzoli, T. Di Girolamo, G. Di Sciascio, C.F. Feng

TL;DR
This study analyzed eight years of ARGO-YBJ data to search for GeV gamma-ray bursts coinciding with satellite detections, setting upper limits on fluence due to no significant detections.
Contribution
First large ground-based analysis of 206 GRBs in the 1-100 GeV range, providing fluence upper limits and constraining spectral extrapolations.
Findings
No significant gamma-ray excess detected.
Fluence upper limits as low as 10^{-5} erg/cm^2.
Constraints on spectral cutoffs for GRBs with known redshift.
Abstract
The search for Gamma Ray Burst (GRB) emission in the energy range 1-100 GeV in coincidence with the satellite detection has been carried out using the Astrophysical Radiation with Ground-based Observatory at YangBaJing (ARGO-YBJ) experiment. The high altitude location (4300 m a.s.l.), the large active surface ( 6700 m of Resistive Plate Chambers), the wide field of view (sr, limited only by the atmospheric absorption) and the high duty cycle ( 86 %) make the ARGO-YBJ experiment particularly suitable to detect short and unexpected events like GRBs. With the scaler mode technique, i.e., counting all the particles hitting the detector with no measurement of the primary energy and arrival direction, the minimum threshold of 1 GeV can be reached, overlapping the direct measurements carried out by satellites. During the experiment lifetime, from December 17, 2004…
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