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Kilodegree Extremely Little Telescope : ウィキペディア英語版
Kilodegree Extremely Little Telescope

The Kilodegree Extremely Little Telescope (or KELT) consists of two robotic telescopes that are conducting a survey for transiting exoplanets around bright stars. The project is jointly administered by members of the Ohio State University Department of Astronomy, the Vanderbilt University Department of Physics and Astronomy Astronomy Group, the Lehigh University Department of Physics, and the South African Astronomical Observatory (SAAO).
== KELT Telescopes ==

KELT consists of two telescopes, KELT-North in Arizona in the United States, and KELT-South at the SAAO observing station near Sutherland, South Africa.
Each KELT telescope consists of a wide field (26 degrees by 26 degrees) medium format telephoto lens with a 4.2 cm aperture, mounted in from of a 4k x 4k Apogee CCD. KELT-North uses an Apogee AP16E camera, while KELT South uses an Apogee U16M. The optical assemblies and cameras are mounted on Paramount ME mounts manufactured by Software Bisque.

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