Investigation of the seeing for the 2-m telescope at Terskol Peak

Details Investigation of the seeing for the 2-m telescope at Terskol Peak Investigation of the seeing for the 2-m telescope at Terskol Peak

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003kfnts...4...75a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 4, p. 75-80

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Scientific paper

We derived the extinction coefficients in the UBVRI bands of the Johnson system, together with the night-sky luminosity, the FWHM function of star images, the distribution of the photomultiplier, the errors of CCD-photometry, as well as other data calculated from extensive observations in 1985-1991 and 1997 with the telescopes mounted on Terskol Peak. The specially arranged observations obtained in 1998-2001 with the 2-m telescope equipped with a Hartmann diaphragm allowed us to study the seeing contribution of the tube and of the air mass inside the dome, to estimate star image quality, and to make recommendations how to reach the limiting resolution of the 2-m telescope.

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