Published September 2008 | Version v1
Miscellaneous

Search for emission from Gamma Ray Bursts with the ARGO-YBJ detector

  • 1. ARGO-YBJ Collaboration and Universita di Napoli 'Federico II' and INFN, Dipartimento di Scienze Fisiche, Complesso Universitario Monte S. Angelo, Via Cintia, 80126 Napoli (Italy)

Description

ARGO-YBJ is a full coverage air shower detector consisting of a 6700 m2 carpet of Resistive Plate Counters, located at Yangbajing (Tibet, P.R.China, 4300 m a.s.l.). Its large field of view (∼ 2 sr) makes ARGO-YBJ particularly suitable to detect unpredictable and short duration events such as Gamma Ray Bursts. ARGO-YBJ works using two techniques: the Scaler Mode, which reaches the lower energy limit (∼ 1 GeV ) of the detector, and the Shower Mode, with an energy threshold of a few hundreds of GeV. Here we present the results of the search for emission from Gamma Ray Bursts in coincidence with satellite detections. (authors)

Part of:
Proceedings of the 21. European Cosmic Ray Symposium

Additional details

Identifiers

Publishing Information

Publisher
Institute of Experimental Physics, Slovak Academy of Sciences
Imprint Place
Kosice (Slovakia)
ISBN
978-80-968060-5-8
Imprint Title
Proceedings of the 21. European Cosmic Ray Symposium
Imprint Pagination
634 p.
Journal Page Range
p. 600-604
Report number
INIS-SK--2010-040

Conference

Title
21. European Cosmic Ray Symposium
Dates
9-12 Sep 2008
Place
Kosice (Slovakia)

Optional Information

Notes
6 figs., 21 refs.