Volume 334, Issue 8 pp. 828-831
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Expected characteristics of data from the LYRA mission

A.I. Zakharov

Corresponding Author

A.I. Zakharov

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, Russia

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, RussiaSearch for more papers by this author
A.V. Mironov

A.V. Mironov

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, Russia

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M.E. Prokhorov

M.E. Prokhorov

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, Russia

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F.N. Nikolaev

F.N. Nikolaev

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, Russia

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M.S. Tuchin

M.S. Tuchin

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, Russia

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A.V. Biryukov

A.V. Biryukov

Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect 13, 119991 Moscow, Russia

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First published: 01 October 2013
Citations: 1

Abstract

The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3m to 16m from the International Space Station, to result in a high-precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001–0.003m for stars brighter than 12m and 0.01m for the stars down to 16m. The estimated duration of the survey is about 5 years. This paper describes the characteristics of data to be received in the course of the LYRA experiment for future users. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

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