Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/12446
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dc.contributor.authorSmith, A.en
dc.contributor.authorPace, R.en
dc.contributor.authorEdwards, P.en
dc.contributor.authorClay, R.en
dc.date.issued1995en
dc.identifier.citationAstrophysics and Space Science, 1995; 231(1-2):319-322en
dc.identifier.issn0004-640Xen
dc.identifier.issn1572-946Xen
dc.identifier.urihttp://hdl.handle.net/2440/12446-
dc.description© 1995 Kluwer Academic Publishersen
dc.description.abstractOf great importance in distinguishing between models for gamma-ray bursts (GRBs) is the experimental determination of the highest energy gamma rays associated with bursts. The EGRET detection of a 15 GeV gamma ray indicates that the spectra of at least some bursts extend well beyond the several MeV limit of the BATSE detectors (Hurleyet al., 1994). The low expected flux means that the collecting area of the present generation of satellite-based detectors is too small to detect gamma rays much above this energy efficiently, and such searches are currently undertaken with ground based detectors. In this paper searches made for very high energy GRBs with a southern hemisphere air shower particle array are described.en
dc.description.statementofresponsibilityA. G. K. Smith, R. W. Clay, R. T. Pace, R. J. Protheroe and P. G. Edwardsen
dc.language.isoenen
dc.publisherKluweren
dc.titleA search for very high energy burstsen
dc.typeJournal articleen
dc.identifier.doi10.1007/BF00658641en
pubs.publication-statusPublisheden
dc.identifier.orcidClay, R. [0000-0002-9040-9648]en
Appears in Collections:Physics publications

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