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Observations of low energy gamma-ray bursts with SAS-2

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Abstract

Low energy celestial gamma ray bursts were discovered1 in 1973 and the detection later confirmed by several groups. In this paper we report the low energy gamma-ray bursts ob served by the plastic scintillator anticoincidence dome of the Small Astronomy Satellite-2 (SAS-2) gamma-ray telescope. Although the high energy gamma-ray telescope of SAS-2 has a threshold of about 20 MeV the large SAS-2 anti coincidence dome (A-dome) which is the outermost element of the instrument provides a very large detector for the high energy portion (⩾0.3 MeV) of these burst events.

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References

  1. Klebesadel, R. W., Strong, I. B., and Olsen, R. A., Astrophys. J. Lett., 182, L85 (1973).

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  2. Derdeyn, S. M., Ehrmann, C. H., Fichtel, C. E., Kniffen, D. A., and Ross, R. W., Nucl. Instrum. Meth., 98, 557 (1972).

    Article  ADS  CAS  Google Scholar 

  3. Strong, I. B., Klebesadel, R. W., and Olsen, R. A., Astrophys. J. Lett., 188, L1 (1974).

    Article  ADS  Google Scholar 

  4. Imhof, W. L., et al., Astrophys. J. Lett., 191, L7 (1974).

    Article  ADS  Google Scholar 

  5. Cline, T. L., and Desai, U. D., Astrophys. J., 195 (in the press).

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ÖGELMAN, H., FICHTEL, C. & KNIFFEN, D. Observations of low energy gamma-ray bursts with SAS-2. Nature 255, 208–210 (1975). https://doi.org/10.1038/255208b0

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  • DOI: https://doi.org/10.1038/255208b0

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