Master Robotic Net
V. LipunovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991V. KornilovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991E. GorbovskoySternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991Nikolaj ShatskijSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991D. KuvshinovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991Nataly TyurinaSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991A. BelinskiSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991Alexander KrylovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991P. BalanutsaSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991V. ChazovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991A. KuznetsovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991Petr KortunovSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991A. SankovichSternberg Astronomical Institute, Moscow State University, 13 Univeristetskij pr-t, Moscow 119991A. TlatovA. ParkhomenkoV. KrushinskyIvan ZalozhnyhA. PopovTaisia KopytovaКирилл ИвановIrkutsk State University, 1 Karl Marks ul., Irkutsk 664003S. YazevIrkutsk State University, 1 Karl Marks ul., Irkutsk 664003V. YurkovBlagoveschensk State Pedagogical University, 104 Lenina street, Blagoveschensk 675000, Amur region
2010en
ABI
Аннотация
The main goal of the MASTER‐Net project is to produce a unique fast sky survey with all sky observed over a single night down to a limiting magnitude of 19‐20. Such a survey will make it possible to address a number of fundamental problems: search for dark energy via the discovery and photometry of supernovae (including SNIa), search for exoplanets, microlensing effects, discovery of minor bodies in the Solar System, and space‐junk monitoring. All MASTER telescopes can be guided by alerts, and we plan to observe prompt optical emission from gamma‐ray bursts synchronously in several filters and in several polarization planes.
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