Gamma ray bursts monitoring with the ARGO-YBJ experiment in scaler mode T. Di Girolamo1, P. Vallania2, and C. Vigorito3 1University of Napoli and INFN-Napoli, Complesso Universitario di Monte Sant'Angelo, via Cinthia, 80126 Napoli, Italy 2IFSI-Torino, INAF and INFN-Torino, corso Fiume 4,10133 Torino, Italy 3University of Torino and INFN Torino, via Pietro Giuria 1, 10125, Torino Italy
Received: 26 Oct 2010 – Revised: 24 Jan 2011 – Accepted: 25 Jan 2011 – Published: 04 Jul 2011
Abstract. We report on the search for Gamma Ray Bursts (GRBs) in the energy range
1–100 GeV in coincidence with the prompt emission detected by satellites,
using the Astrophysical Radiation Ground-based Observatory at YangBaJing
(ARGO-YBJ).
With its big active surface (~6700 m2) and large field of view
(≥2 sr) the ARGO-YBJ air shower detector is particularly suitable to
detect unpredictable and short duration events such as GRBs.
The search has been performed using the single particle technique in
time coincidence with satellite detections
both for single events and for the
piling up of all the GRBs in time and in phase.
Between November 2004 and June 2010
115 GRBs, detected by different satellites (mainly Swift and Fermi),
occurred within the field of view of ARGO-YBJ.
For 94 of these we searched
for a counterpart in the ARGO-YBJ data finding no
statistically significant emission.
Search methods and results are discussed.
Citation: Di Girolamo, T., Vallania, P., and Vigorito, C.: Gamma ray bursts monitoring with the ARGO-YBJ experiment in scaler mode, Astrophys. Space Sci. Trans., 7, 239-243, doi:10.5194/astra-7-239-2011, 2011.