{ "id": "1605.04274", "version": "v1", "published": "2016-05-13T18:10:57.000Z", "updated": "2016-05-13T18:10:57.000Z", "title": "Prompt emission from GRB 150915A in the GeV energy range detected at ground by the New-Tupi detector", "authors": [ "C. R. A. Augusto", "C. E. Navia", "M. N. de Oliveira", "A. A. Nepomuceno", "V. Kopenkin", "T. Sinzi" ], "comment": "9 pages, 9 figures", "categories": [ "astro-ph.HE" ], "abstract": "Since 2014, a new detector (New-Tupi) consisting of four plastic scintillators ($150 \\times 75 \\times 5 cm^3$) placed in pairs and located in Niteroi, Rio de Janeiro, Brazil, has been used for the search of transient solar events and photomuons from gamma-ray bursts (GRBs). On September 15, 2015, at 21:18:24 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 150915A (trigger 655721). The GRB light curve shows a weak complex structure of long duration $T_{90}=164.7 \\pm 49.7 $ sec, and a fluence in the 15-150 keV band of $8.0 \\pm 1.8 \\times 10^{-7}erg/cm^2$. GRB 150915A was fortuitously located in the field of view of the New-Tupi detector, and a search for prompt emission in the GeV energy range is presented here. The analysis was made using the \"scaler\" or \"single-particle\" technique. The New-Tupi detector registered a muon excess peak of 6.1s duration with a signal significance $6.9\\sigma$, the signal was within the T90 duration of the Swift BAT GRB, with an estimated fluence $4.8 \\times 10^{-6} erg/cm^2$ (10-100 GeV). The Poisson probability of the event to be a background fluctuation is $6.9 \\times 10^{-10}$ and it appears in the counting rate of the New-Tupi detector with an annual rate $\\sim 2.6$.", "revisions": [ { "version": "v1", "updated": "2016-05-13T18:10:57.000Z" } ], "analyses": { "keywords": [ "gev energy range", "new-tupi detector", "grb 150915a", "prompt emission", "swift burst alert telescope" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1458941 } } }