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Gamma Ray Bursts Monitoring with the Argo-ybj Experiment in Scaler Mode : Volume 7, Issue 3 (04/07/2011)

By Di Girolamo, T.

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Book Id: WPLBN0004002773
Format Type: PDF Article :
File Size: Pages 5
Reproduction Date: 2015

Title: Gamma Ray Bursts Monitoring with the Argo-ybj Experiment in Scaler Mode : Volume 7, Issue 3 (04/07/2011)  
Author: Di Girolamo, T.
Volume: Vol. 7, Issue 3
Language: English
Subject: Science, Astrophysics, Space
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Historic
Publication Date:
2011
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

Citation

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Vallania, P., Girolamo, T. D., & Vigorito, C. (2011). Gamma Ray Bursts Monitoring with the Argo-ybj Experiment in Scaler Mode : Volume 7, Issue 3 (04/07/2011). Retrieved from http://www.ebooklibrary.org/


Description
Description: University of Napoli and INFN-Napoli, Complesso Universitario di Monte Sant'Angelo, via Cinthia, 80126 Napoli, Italy. 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.


Summary
Gamma ray bursts monitoring with the ARGO-YBJ experiment in scaler mode

Excerpt
Aglietta, M., et al. (EASTOP collaboration): Search for γ ray bursts at photon energies $E_0 \geq 10$ GeV and $E_0 \geq 80$ TeV, Astrophys. J., 469, 305 – 310, 1996.; Aielli, G., et al. (ARGO-YBJ collaboration): Layout and performance of RPCs used in the Argo-YBJ experiment, Nucl. Instr. Meth. A, 562, 92 – 96, 2006.; Aielli, G., et al. (ARGO-YBJ collaboration): Scaler mode technique for the ARGO-YBJ detector, Astropart. Phys., 30, 85 – 95, 2008.; Aielli, G., et al. (ARGO-YBJ collaboration): Search for Gamma Ray Bursts with th ARGO-YBJ detector in scaler mode, Astrophys. J., 699, 1281 – 1287, 2009a.; Aielli, G., et al. (ARGO-YBJ collaboration): ARGO-YBJ constraints on very high energy emission from GRBs, Astropart. Phys., 32, 47 – 52, 2009b.; Albert, J., et al. (MAGIC collaboration): MAGIC uppper limits on the very high energy emission from Gamma-Ray Bursts, Astrophys. J., 667, 358 – 366, 2007.; Alexandreas, D. E., Allen, G. E., Berkley, D., et al.: Search for ultra-high-energy radiation from gamma-ray bursts, Astrophys. J. 426, 1 – 3, 1994.; Castellina, A., et al. (INCA collaboration): Search for GeV gamma ray bursts at Mount Chacaltaya, in: Proc. 27th ICRC, 2735 – 2738, 2001.; Dingus, B. L., Catelli, J. R., and Schneid, E. J.: EGRET fluxes and upper limits for energetic gamma ray bursts, in: Proc. 25th ICRC, 3, 33 – 36, 1997.; Helene, O.: Upper limit of peak area, Nucl. Instr. Meth., 212, 319 – 322, 1983.; Kneiske, T. M., Bretz, T., Mannheim, K., et al.: Implications of cosmological gamma-ray absorption, Astron. Astrophys., 413, 807 – 815, 2004.; Li, T. and Ma, Y.: Analysis methods for results in gamma-ray astronomy, Astrophys. J., 272, 317 – 327, 1983.; Morello, C., Navarra, G., and Periale, L.: A search for high-energy cosmic gamma-ray bursts, Il Nuovo Cimento, 7C, 682 – 688, 1984.; O'Brian, S. and Porter, N. A.: Upper limits for high energy γ-rays in association with Vela bursts, Astrophys. Space Science, 42, 73 – 76, 1976.

 

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