The Kilodegree Extremely Little Telescope (KELT): A Small Robotic Telescope for Large‐Area Synoptic Surveys

@article{Pepper2007TheKE,
  title={The Kilodegree Extremely Little Telescope (KELT): A Small Robotic Telescope for Large‐Area Synoptic Surveys},
  author={Joshua A. Pepper and Richard W. Pogge and Darren Lee Depoy and Jennifer L. Marshall and Krzysztof Zbigniew Stanek and Amelia M. Stutz and Shawn Poindexter and Robert J. Siverd and Thomas Paul O'Brien and Mark Trueblood and Patricia Trueblood The Ohio State University Department of Astronomy and University of Arizona Department of Astronomy and Winer Observatory},
  journal={Publications of the Astronomical Society of the Pacific},
  year={2007},
  volume={119},
  pages={923-935}
}
ABSTRACT 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 \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs… 
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References

SHOWING 1-10 OF 24 REFERENCES
HATnet VARIABILITY SURVEY IN THE HIGH STELLAR DENSITY "KEPLER FIELD" WITH MILLIMAGNITUDE IMAGE SUBTRACTION PHOTOMETRY
The Hungarian-made Automated Telescope network (HATnet) is an ongoing project to detect transiting extra-solar planets using small aperture (11 cm diameter), robotic telescopes. In this paper we
HAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting One Member of a Stellar Binary* **
Using small automated telescopes in Arizona and Hawaii, the HATNet project has detected an object transiting one member of the double star system ADS 16402. This system is a pair of G0 main-sequence
Using All-Sky Surveys to Find Planetary Transits
Transits of bright stars offer a unique opportunity to study detailed properties of extrasolar planets that cannot be determined through radial-velocity observations. We propose a new technique to
TrES-1: The Transiting Planet of a Bright K0 V Star
We report the detection of a transiting Jupiter-sized planet orbiting a relatively bright (V = 11.79) K0 V star. We detected the transit light-curve signature in the course of the TrES multisite
Transit Detectability of Ring Systems around Extrasolar Giant Planets
We investigate whether rings around extrasolar planets could be detected from those planets' transit light curves. To this end, we develop a basic theoretical framework for calculating and
The effect of red noise on planetary transit detection
Since the discovery of short-period exoplanets a decade ago, photometric surveys have been recognized as a feasible method to detect transiting hot Jupiters. Many transit surveys are now underway,
DAOPHOT: A Computer Program for Crowded-Field Stellar Photometry
The tasks of the DAOPHOT program, developed to exploit the capability of photometrically linear image detectors to perform stellar photometry in crowded fields, are discussed. Raw CCD images are
Detection of an Extrasolar Planet Atmosphere
We report high-precision spectrophotometric observations of four planetary transits of HD 209458, in the region of the sodium resonance doublet at 589.3 nm. We find that the photometric dimming
A Technique for Ultrahigh‐Precision CCD Photometry
We present techniques for wide-field ultrahigh-precision time-sampled CCD photometry. Representing a survey of field stars, our data consist of UBVRI photometry and a V-band time series of exposures
THE INTERIORS OF GIANT PLANETS: Models and Outstanding Questions
▪ Abstract We know that giant planets played a crucial role in the making of our Solar System. The discovery of giant planets orbiting other stars is a formidable opportunity to learn more about
...
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