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The BDRG and SHOK instruments for studying gamma-ray burst prompt emission onboard the Lomonosov spacecraft

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Abstract

One of the goals of the Lomonosov satellite designed by scientists of Moscow State University is to study the prompt emission of cosmic gamma-ray bursts. This paper describes the gamma-ray burst monitor in the gamma-ray range (the BDRG instrument) and the wide-field optical cameras (the SHOK instrument) for detecting both the gamma-ray burst prompt emission and its precursors.

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References

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Correspondence to S. I. Svertilov.

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Original Russian Text © A.M. Amelyushkin, V.I. Galkin, B.V. Goncharov, E.S. Gorbovskoy, V.G. Kornilov, V.M. Lipunov, M.I. Panasyuk, V.L. Petrov, G.F. Smoot, S.I. Svertilov, N.N. Vedenkin, I.V. Yashin, 2013, published in Kosmicheskie Issledovaniya, 2013, Vol. 51, No. 6, pp. 478–483.

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Amelyushkin, A.M., Galkin, V.I., Goncharov, B.V. et al. The BDRG and SHOK instruments for studying gamma-ray burst prompt emission onboard the Lomonosov spacecraft. Cosmic Res 51, 434–438 (2013). https://doi.org/10.1134/S0010952513060014

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  • DOI: https://doi.org/10.1134/S0010952513060014

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