• Mayor M., Sahlmann J., Martin E.L., et al.Differential image motion in astrometric observations with very large seeing- limited telescopes. 2024,A&A,Vol.689A,p. A94 (17 pp.). 2024A&A...689A..94L
  • Raddi R., Burgasser A. J., Casewell S. L., et al.Primeval very low-mass stars and brown dwarfs - VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf. 2024,MNRAS,V.533,is.2,p.1654-1669. 2024MNRAS.533.1654Z
  • Dobrycheva D.V., Pavlenko Ya.V., Luk'yanyk I., et al.Numerical simulations of exocomet transits: Insights from β Pic and KIC 3542116. 2024,A&A,Vol.688A,p.65 (9 pp.). 2024A&A...688A..65L
  • Ishchenko M.V., Sobolenko M., Berczik P.,Dynamical evolution timescales for the triple supermassive black hole system in NGC 6240. 2024,A&A,Vol.687L,p.18 (13 pp.). 2024A&A...687L..18B
  • Shubina O.S., Zubko E., Husárik M., et al.Dust properties and their variations in comet C/2013 X1 (PANSTARRS). 2024,A&A,Vol.687A,p.297 (12 pp.). 2024A&A...687A.297S
  • Paolillo M., Carrera F. J., Civano F., et al.Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low- redshift galaxies. 2024,MNRAS,Vol.527,is.4,p.12091-12108. 2024MNRAS.52712091T

 

 

 

 

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Astrographs

The Tepfer–Steingel double astrograph

The Tepfer double astrograph (D=40 cm, F=550 cm) one of the first instruments installed at the Golosiiv site (1946). It is used for studying stellar proper motions, structure of the Galaxy, positions of the Solar System bodies, and Moon study. Observations are carried out in the International B, V system, down to 15m. A new dome for the double long-focus astrograph was completed in 1991.

The Tepfer–Steingel double astrograph

The Zeiss double wide-angle astrograph

The Zeiss double wide-angle astrograph (D = 40 cm, F = 200 cm) was mounted in 1975. The limiting photographic magnitude is 16m. Planets, asteroids, and comets are observed with this instrument for compiling different catalogues. Plates obtained with this telescope are used for the Northern Sky Survey (FON).

The Zeiss double wide-angle astrograph