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Abstrakty
We propose an improved method for the atmospheric extinction reduction within optical photometry. Our method is based on the simultaneous multicolor observations of photometric standards. Such data are now available within the modern wide-field sky surveys and contain a large amount of information about instant atmospheric conditions. So, it became possible to estimate the extinction parameters on the basis of a quite short observational dataset and, hence, to trace the rapid stars twinkling accurately. Having been developed for a new MiniMegaTORTORa observational system, the proposed method can be adopted for a wide range of modern observational programs.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
197--204
Opis fizyczny
Bibliogr. 22 poz., wykr.
Twórcy
autor
- Sternberg Astronomical Institute of M.V. Lomonosov Moscow State University, 13 Universitetsky pr., Moscow, 119991 Russia
autor
- Sternberg Astronomical Institute of M.V. Lomonosov Moscow State University, 13 Universitetsky pr., Moscow, 119991 Russia
autor
- Sternberg Astronomical Institute of M.V. Lomonosov Moscow State University, 13 Universitetsky pr., Moscow, 119991 Russia
- Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
autor
- Sternberg Astronomical Institute of M.V. Lomonosov Moscow State University, 13 Universitetsky pr., Moscow, 119991 Russia
autor
- Sternberg Astronomical Institute of M.V. Lomonosov Moscow State University, 13 Universitetsky pr., Moscow, 119991 Russia
autor
- Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
- Special Astrophysical Observatory, Karachai-Cherkessia, Nizhnij Arkhyz, 369167 Russia
autor
- Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
- Special Astrophysical Observatory, Karachai-Cherkessia, Nizhnij Arkhyz, 369167 Russia
autor
- Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
- Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
- Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
- Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
- Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
Bibliografia
- Beskin, G., et al. 2013, Phys. Usp., 56, 836.
- Bessel, M.S. 1990, PASP, 102, 1181.
- Biryukov, A., Beskin, G., Karpov, S., Bondar, S., Ivanov, E., Katkova, E., Perkov, A., and Sasyuk, V. 2015, Baltic Astronomy, 24, 100.
- Dravins, D., Lindegren, L., Mezey, E., and Young, A.T. 1997, PASP, 109, 173.
- Fitzpatrick, E. 1999, PASP, 111, 63.
- Gershberg, R.E. 2005, “Solar-Type Activity in Main-Sequence Stars”, Heidelberg, Springer.
- Ivezic, Z., et al. 2008, Serbian Astronomical Journal, 176, 1.
- Johnson, H.L., and Morgan, W.W. 1953, ApJ, 117, 313.
- Kaiser, M., et al. 2002, in: “Survey and Other Telescope Technologies and Discoveries”. Eds., Tyson, J., and Wolff, A., Proceedings of the SPIE, 4836, p. 154.
- Kasting, J.F., Whitmire, D.P., and Reynolds, R.T. 1993, Icarus, 101, 108.
- Kornilov, V., et al. 1991, Trans. of the Sternberg Astronomical Institute (in Russian), 63.
- Kornilov, V., Mironov, A., and Zakharov, A. 1996, Baltic Astronomy, 5, 379.
- Kornilov, V. 1998, Baltic Astronomy, 7, 513.
- Kroussanova, N., Mironov, A.V., and Zakharov,A.I. 2013, Peremennye Zvezdy, 33, 8.
- Lindegren, L., and Perryman, M.A.C. 1996, A&AS, 116, 579.
- Lipunov, V., et al. 2010, Advances in Astronomy, 2010, 30.
- Maehara, H., et al. 2012, Nature, 485, 478.
- Pickles, A.J. 1998, PASP, 110, 863.
- Pojmański, G. 1997, Acta Astronomica, 47, 467.
- Quintana, E.V., et al. 2014, Science, 344, 277.
- Straizys, V. 1992, “Multicolor Stellar Photometry”, Astron. and Astrophys. Ser., p. 15.
- Straizys, V. 1999, Baltic Astronomy, 8, 505.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-b7847ed3-b5a8-4ba2-a416-5ea9b26c6b31