MASTER global robotic net

V. Lipunov1,2, V. Kornilov1, E. Gorbovskoy1,2, A. Belinski1, D. Kuvshinov1, N. Tyurina1, A. Krylov1, N. Shatsky1, P. Balanutsa1, V. Chazov1, A. Kuznetsov1, D. Zimnuhov1, A. Tlatov3, A. Parkhomenko3, D. Dormidontov3, V. Krushinsky4, I. Zalozhnyh4, A. Popov4, S. Yazev5, N. Budnev5, K. Ivanov5, E. Konstantinov5, O. Gress5, O. Chvalaev5, V. Yurkov6, Y. Sergienko6, I. Kudelina6
1Sternberg Astronomical Institute of Moscow State University, Moscow
2"Extreme Universe" Laboratory of Lomonosov Moscow State University of Skobeltsyn Institute of Nuclear Physics, Moscow
3Kislovodsk Solar Station of the Pulkovo Observatory, Kislovodsk
4Ural Federal University, Kourovka observatory
5,6Blagoveschensk Educational State University, Blagoveschensk

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Abstract

The paper presents the basic principles of the design of the robotic network of optical telescopes MASTER, developed to study the prompt optical emission of gamma-ray bursts. The robotic telescopes MASTER II near Kislovodsk, Ekaterinburg, Irkutsk and Blagoveshchensk were installed and started to operate, thanks to the support of Sternberg astronomical institute, High altitude astronomical station of the Pulkovo observatory, Ural state university, Irkutsk state university, Blagoveshchensk pedagogical university. The network span over the longitudes is greater than 6 hours.



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Keywords : robotic observations – GRB – transients – Supernovae