Search Results - (Author, Cooperation:P. G. Edwards)
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1L. A. T. C. Fermi ; M. Ackermann ; M. Ajello ; J. Ballet ; G. Barbiellini ; D. Bastieri ; A. Belfiore ; R. Bellazzini ; B. Berenji ; R. D. Blandford ; E. D. Bloom ; E. Bonamente ; A. W. Borgland ; J. Bregeon ; M. Brigida ; P. Bruel ; R. Buehler ; S. Buson ; G. A. Caliandro ; R. A. Cameron ; P. A. Caraveo ; E. Cavazzuti ; C. Cecchi ; O. Celik ; E. Charles ; S. Chaty ; A. Chekhtman ; C. C. Cheung ; J. Chiang ; S. Ciprini ; R. Claus ; J. Cohen-Tanugi ; S. Corbel ; R. H. Corbet ; S. Cutini ; A. de Luca ; P. R. den Hartog ; F. de Palma ; C. D. Dermer ; S. W. Digel ; E. do Couto e Silva ; D. Donato ; P. S. Drell ; A. Drlica-Wagner ; R. Dubois ; G. Dubus ; C. Favuzzi ; S. J. Fegan ; E. C. Ferrara ; W. B. Focke ; P. Fortin ; Y. Fukazawa ; S. Funk ; P. Fusco ; F. Gargano ; D. Gasparrini ; N. Gehrels ; S. Germani ; N. Giglietto ; F. Giordano ; M. Giroletti ; T. Glanzman ; G. Godfrey ; I. A. Grenier ; J. E. Grove ; S. Guiriec ; D. Hadasch ; Y. Hanabata ; A. K. Harding ; M. Hayashida ; E. Hays ; A. B. Hill ; R. E. Hughes ; G. Johannesson ; A. S. Johnson ; T. J. Johnson ; T. Kamae ; H. Katagiri ; J. Kataoka ; M. Kerr ; J. Knodlseder ; M. Kuss ; J. Lande ; F. Longo ; F. Loparco ; M. N. Lovellette ; P. Lubrano ; M. N. Mazziotta ; J. E. McEnery ; P. F. Michelson ; W. Mitthumsiri ; T. Mizuno ; C. Monte ; M. E. Monzani ; A. Morselli ; I. V. Moskalenko ; S. Murgia ; T. Nakamori ; M. Naumann-Godo ; J. P. Norris ; E. Nuss ; M. Ohno ; T. Ohsugi ; A. Okumura ; N. Omodei ; E. Orlando ; M. Ozaki ; D. Paneque ; D. Parent ; M. Pesce-Rollins ; M. Pierbattista ; F. Piron ; G. Pivato ; T. A. Porter ; S. Raino ; R. Rando ; M. Razzano ; A. Reimer ; O. Reimer ; S. Ritz ; R. W. Romani ; M. Roth ; P. M. Saz Parkinson ; C. Sgro ; E. J. Siskind ; G. Spandre ; P. Spinelli ; D. J. Suson ; H. Takahashi ; T. Tanaka ; J. G. Thayer ; J. B. Thayer ; D. J. Thompson ; L. Tibaldo ; M. Tinivella ; D. F. Torres ; G. Tosti ; E. Troja ; Y. Uchiyama ; T. L. Usher ; J. Vandenbroucke ; G. Vianello ; V. Vitale ; A. P. Waite ; B. L. Winer ; K. S. Wood ; M. Wood ; Z. Yang ; S. Zimmer ; M. J. Coe ; F. Di Mille ; P. G. Edwards ; M. D. Filipovic ; J. L. Payne ; J. Stevens ; M. A. Torres
American Association for the Advancement of Science (AAAS)
Published 2012Staff ViewPublication Date: 2012-01-17Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Staff View
ISSN: 0022-0094Topics: HistoryPolitical ScienceURL: -
3Tanimori, T. ; Naito, T. ; Yoshida, T. ; Yanagita, S. ; Mori, M. ; Edwards, P. G. ; Asahara, A. ; Bicknell, G. V. ; Gunji, S. ; Hara, S. ; Hara, T. ; Hayashi, S. ; Itoh, C. ; Kabuki, S. ; Kajino, F. ; Katagiri, H. ; Kataoka, J. ; Kawachi, A. ; Kifune, T. ; Kubo, H. ; Kushida, J. ; Maeda, S. ; Maeshiro, A. ; Matsubara, Y. ; Mizumoto, Y.
[s.l.] : Macmillian Magazines Ltd.
Published 2002Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Protons with energies up to ∼1015 eV are the main component of cosmic rays, but evidence for the specific locations where they could have been accelerated to these energies has been lacking. Electrons are known to be accelerated to cosmic-ray energies in supernova ...Type of Medium: Electronic ResourceURL: -
4Smith, A. G. K. ; Clay, R. W. ; Pace, R. T. ; Protheroe, R. J. ; Edwards, P. G.
Springer
Published 1995Staff ViewISSN: 1572-946XKeywords: Gamma ray bursts ; ObservationsSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract Of 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.Type of Medium: Electronic ResourceURL: