Primary corrector of Japanese National Large Telescope (JNLT)

Details Primary corrector of Japanese National Large Telescope (JNLT) Primary corrector of Japanese National Large Telescope (JNLT)

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990spie.1236..125n&link_type=abstract

IN: Advanced technology optical telescopes IV; Proceedings of the Meeting, Tucson, AZ, Feb. 12-16, 1990. Part 1 (A91-23201 08-89

Astronomy and Astrophysics

Astronomy

Error Correcting Devices, Field Of View, Seeing (Astronomy), Telescopes, Visible Spectrum, Image Processing, Japan, Lenses, Mirrors, Optical Properties, Refractivity

Scientific paper

At the primary focus of JNLT, three-lens correctors with two aspheric surfaces will be used. They are designed for the wavelength region of 320-500 nm and 440-1100 nm, respectively, and provide images of less than 0.2 arcsec rms radius for a field of 30 arcmin diameter. The corrector for the blue region will include an atmospheric dispersion corrector. Characteristics of aberrations that arises in JNLT primary corrector are discussed.

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