The atmospheric dispersion coefficient of the objectives of the double long-focus astrograph and double wide-angle astrograph of the Main Astronomical Observatory in Kiev.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astrographs: Star Positions, Astrographs: Astrometry

Scientific paper

The atmospheric dispersion coefficients of double long-focus astrograph and double wide-angle astrograph objectives are determined for spectral intervals A-G, A-F, F-G and different magnitudes. The coefficients strongly depend on the brightness of the star and to a less extent depend on the spectral interval width. The atmospheric dispersion influences the positions of stars brighter than 10m.

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