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    Results of a Three Year Search for Bursts of High Energy Gamma Rays Using Widely Spaced Cosmic Ray Stations
    International Cosmic Ray Conference (1979)
    D. J. FeganB. McBreenColm O’Sullivan
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    Keywords:
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    Average Cosmological Invariant Parameters of Cosmic Gamma‐Ray Bursts
    The Astrophysical Journal (1999)
    И. Г. МитрофановD. AnfimovM. L. LitvakM. S. BriggsW. S. Pačiesas
    Average cosmological invariant parameters (ACIPs) are calculated for six groups of BATSE cosmic gamma-ray bursts selected by their peak fluxes on the 1.024 s timescale. The ACIPs represent the average temporal and spectral properties of these events equally in the observer frame of reference and in the comoving frames of outbursting emitters. The parameters are determined separately for rise fronts and for back slopes of bursts, defined as the time profiles before and after the main peaks, respectively. The ACIPs for the rise fronts are found to be different for different intensity groups, while the ACIPs for the back slopes show no significant dependence on intensity. We conclude that emitters of bursts manifest standard average properties only during the back slopes of bursts.
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    A search for very high energy bursts
    Astrophysics and Space Science (1995)
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    No new limit on the size distribution of gamma-ray bursts
    NASA STI/Recon Technical Report N (1976)
    T. ClineW. Schmidt
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    Upper limit for the number of gamma-ray bursts in 2 - 25 keV energy range from satellite data of the Astron.
    Kosmicheskie Issledovaniia (1999)
    V. G. KurtE. K. Sheffer
    Astron
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    Observations of cosmic gamma ray bursts with WATCH on EURECA
    Advances in Space Research (1995)
    S. BrandtN. LundA. J. Castro‐Tirado
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    Radio radiation of cosmic gamma-ray bursts.
    Izvestiia Vysshaia Uchebn. Zaved., Radiofizika (1985)
    L. P. GorbachevA. Yu. Matronchik
    Space Radiation
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    The gamma-ray bursts and the cosmic-ray sources
    MmSAI (1996)
    Wolfgang Kundt
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    Measurement of the rate of weak gamma-ray bursts
    AIP conference proceedings (1984)
    C. MeeganG. J. FishmanRichard B. Wilson
    A sensitive search for weak gamma‐ray bursts was conducted using data from two balloon flights. One burst was observed in 64 hours of observation. A 95% confidence upper limit to the burst rate is 2600 bursts/year with fluence greater than 4.4×10−7 ergs/cm2.
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    A search for ultra high-energy γ-ray bursts from celestial sources
    Nature (1980)
    P. N. BhatN. V. GopalakrishnanS. K. GuptaP. V. Ramana MurthyB. V. Sreekantan
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