Abstract
We have determined the realistic seeing of the 1.5-m AZT-22 telescope of the Mt. Maidanak Observatory (Astronomical Institute, Uzbek Academy of Sciences) using more than 20 000 CCD frames with stellar images in the UBV RI bands acquired in 1996–2005: ε = 1.065″ in the V band. The characteristic seeing reduced to unit air mass, ε V med (M(z) = 1), is 0.945″. We derived color equations for the CCD detectors used with the telescope. Atmospheric-extinction coefficients in different photometric bands were also determined. The mean V -band atmospheric extinction is 0.20m ± 0.04m. The time needed for the conditions to settle, in the free atmosphere as well as inside the telescope dome, is 2–2.5 hours after the end of astronomical twilight. For nights with ε V med > 0.9″, we find a persistent difference between the seeing found at this telescope and measured simultaneously with a differential image motion monitor, amounting to ∼0.1m.
Similar content being viewed by others
References
P. V. Shcheglov, Problems of Optical Astronomy (Nauka, Moscow, 1980) [in Russian].
J. Stock, Bull. Astron. 24, 116 (1964).
Yu. N. Efremov, S. B. Novikov, and P. V. Shcheglov, Usp. Fiz. Nauk 115, 301 (1975) [Sov. Phys. Usp. 18, 151 (1975)].
S. A. Potanin, Astron. Zh. 85, 665 (2008) [Astron. Rep. 52, 598 (2008)].
M. V. Lobachev, K. M. Gruzdeva, L. E. Yakukhnova, and K. A. Chernaya, in Methods for Increasing the Efficiency of Optical Telescopes, Ed. by S. A. Gladyshev (Mosk. Gos. Univ., Moscow, 1987), p. 132 [in Russian].
B. P. Artamonov and M. I. Tertitsky, in Methods for Increasing the Efficiency of Optical Telescopes, Ed. by S. A. Gladyshev (Mosk. Gos. Univ., Moscow, 1987), p. 160 [in Russian].
B. P. Artamonov, V. V. Bruevich, O. N. Bugaenko, et al., Preprint Gos. Astron. Inst. Sternberga No. 16 (GAIShMGU, Moscow, 1990).
S. A. Potanin, Astron. Zh. 86, 758 (2009) [Astron. Rep. 53, 703 (2009)].
B. P. Artamonov, S. B. Novikov, and A. A. Ovchinnikov, in Methods for Increasing the Efficiency of Optical Telescopes, Ed. by S. A. Gladyshev (Mosk. Gos. Univ., Moscow, 1987), p. 8 [in Russian].
S. P. Ilyasov, A. K. Baĭzhumanov, M. Saratsin, et al., Pis’ma Astron. Zh. 25, 156 (1999) [Astron. Lett. 25, 122 (1999)].
S. A. Ehgamberdiev, A. K. Baijumanov, S. P. Ilyasov, et al., Astron. Astrophys. Suppl. Ser. 145, 293 (2000).
V. G. Kornilov, S. P. Ilyasov, O. V. Vozyakova, et al., Pis’ma Astron. Zh. 35, 606 (2009) [Astron. Lett. 35, 547 (2009)].
S. B. Novikov and A. A. Ovchinnikov, in Astroclimate and the Efficiency of Telescopes, Ed. by V. S. Shevchenko and A. Kh. Kurmaev (Nauka, Leningrad, 1984), p. 177 [in Russian].
B. P. Artamonov, Proc. SPIE 2871, 737 (1997).
Kh. B. Sultanov, S. P. Il’yasov, and Sh. A. Ehgamberdiev, in Modern Problems of Astronomy in Uzbekistan, Ed. by Sh. A. Ehgamberdiev (AI RUz AS, Tashkent, 2004), p. 21 [in Russian].
V. G. Vakulik, V. N. Dudinov, A. P. Zheleznyak, et al., Astron. Nachr. 318, 73 (1997).
B. P. Artamonov, Yu. Yu. Badan, V. V. Bruevich, and A. S. Gusev, Astron. Zh. 76, 438 (1999) [Astron. Rep. 43, 377 (1999)].
B. P. Artamonov, Yu. Yu. Badan, and A. S. Gusev, Astron. Zh. 77, 643 (2000) [Astron. Rep. 44, 569 (2000)].
M. Sarazin and F. Roddier, Astron. Astrophys. 227, 294 (1990).
T. L. Qian, C. R. Qui, X. F. Cen, et al., Acta Astron. Sinica 42, 101 (2001).
B. Lim, H. Sung, M. S. Bessell, et al., J. Korean Astron. Soc. 42, 161 (2009).
A. S. Gusev, Astron. Zh. 83, 195 (2006) [Astron. Rep. 50, 167 (2006)].
A. S. Gusev, Astron. Zh. 83, 211 (2006) [Astron. Rep. 50, 182 (2006)].
A. U. Landolt, Astron. J. 104, 340 (1992).
G. Petrov, W. Seggewiss, A. Dieball, and B. Kovachev, Astron. Astrophys. 376, 745 (2001).
M. A. Ibragimov, unpublished (2004).
A. P. Zheleznyak, private commun. (2004).
K. Zdanavichyus and D. Matsiyauskas, Byull. Vil’nyussk. Astron. Observ. 55, 11 (1980).
E. Pakstiene, K. Zdanavicius, and S. Bartasiute, Baltic Astron. 10, 651 (2001).
Yu. A. Tillaev, in Modern Problems of Astronomy in Uzbekistan, Ed. by Sh. A. Ehgamberdiev (AI Ruz AS, Tashkent, 2004), p. 34 [in Russian].
Yu. A. Tillaev, S. P. Il’yasov, and K. N. Grankin, Dokl. Akad. Nauk RUz 6, 27 (2004).
W. J. Roberts and E. K. Grebel, Astron. Astrophys. Suppl. Ser. 109, 313 (1995).
A. Jimenez, H. Gonzalez Jorge, and M. C. Rabello-Soares, Astron. Astrophys. Suppl. Ser. 129, 413 (1998).
Author information
Authors and Affiliations
Additional information
Original Russian Text © B.P. Artamonov, V.V. Bruevich, A.S. Gusev, O.V. Ezhkova, M.A. Ibrahimov, S.P. Ilyasov, S.A. Potanin, Yu.A. Tillaev, Sh.A. Ehgamberdiev, 2010, published in Astronomicheskiĭ Zhurnal, 2010, Vol. 87, No. 11, pp. 1106–1119.
Rights and permissions
About this article
Cite this article
Artamonov, B.P., Bruevich, V.V., Gusev, A.S. et al. Seeing and atmospheric extinction at Mt. Maidanak observatory from observations with the 1.5-m AZT-22 telescope. Astron. Rep. 54, 1019–1031 (2010). https://doi.org/10.1134/S1063772910110077
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063772910110077