Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-25T16:43:12.725Z Has data issue: false hasContentIssue false
  • English
  • Français

KELT: A Wide-Field Survey of Bright Stars for Transiting Planets

Published online by Cambridge University Press:  01 May 2008

Robert J. Siverd ,
Joshua Pepper ,
Kris Stanek ,
Richard W. Pogge ,
B. Scott Gaudi  and
Darren L. DePoy
Robert J. Siverd
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH, 43210 email: [email protected], [email protected], [email protected], [email protected], [email protected]
Joshua Pepper
Affiliation:
Vanderbilt University6301 Stevenson Center Nashville, TN 37235 email: [email protected]
Kris Stanek
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH, 43210 email: [email protected], [email protected], [email protected], [email protected], [email protected]
Richard W. Pogge
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH, 43210 email: [email protected], [email protected], [email protected], [email protected], [email protected]
B. Scott Gaudi
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH, 43210 email: [email protected], [email protected], [email protected], [email protected], [email protected]
Darren L. DePoy
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH, 43210 email: [email protected], [email protected], [email protected], [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Kilodegree Extremely Little Telescope (KELT) is a wide-field (26° × 26°) robotic survey telescope currently operating in Sonoita, Arizona. Assembled from commercial and off-the-shelf devices, KELT currently surveys ~40% of the Northern sky with sufficient precision to detect transiting planets around bright (8 < V < 12) stars. In the past several years of operation, over 30,000 science images have been acquired. Planet candidate selection and follow-up are currently underway. A brief overview of past and present survey operations, the data reduction pipeline, and initial results follows below.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 350 - 353
Copyright
Copyright © International Astronomical Union 2009

References

Alard, C. & Lupton, R. H. 1998, ApJ, 503, 325CrossRefGoogle Scholar
Pepper, J., Gould, A., & Depoy, D. L. 2003, AcA, 53, 213Google Scholar
Pepper, J., Stanek, K. Z., Pogge, R. W., Latham, D. W., DePoy, D. L., Siverd, R., Poindexter, S., & Sivakoff, G. R. 2008, AJ, 135, 907CrossRefGoogle Scholar
Pepper, J., Pogge, R. W., DePoy, D. L., Marshall, J. L., Stanek, K. Z., Stutz, A. M., Poindexter, S., Siverd, R., O'Brien, T. P., Trueblood, M., & Trueblood, P. 2007, PASP 119, 923CrossRefGoogle Scholar