2007/04/30 by Joshua Pepper, Richard W. Pogge, Richard W. Pogge +14
Physics and Astronomy · #Astronomy and Astrophysical Research #Space Science and Extraterrestrial Life #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/521836
published as Publ.Astron.Soc.Pac.119:923,2007 · 21 pages, 13 figures; accepted to PASP
arxiv created 2007/07/30 · openalex publication_date 2007/08/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/30
The Kilodegree Extremely Little Telescope (KELT) project is a survey for planetary transits of bright stars. It consists of a small‐aperture, wide‐field automated telescope located at Winer Observatory near Sonoita, Arizona. The telescope surveys a set of 26° × 26° fields that together cover about 25% of the northern sky, and targets stars in the range of 8<V<10 mag, searching for transits by close‐in Jupiters. This paper describes the system hardware and software and discusses the quality of the observations. We show that KELT is able to achieve the necessary photometric precision to detect planetary transits around solar‐type main‐sequence stars.