A 1.1–1.9 GHz SETI SURVEY OF THE KEPLER FIELD. I. A SEARCH FOR NARROW-BAND EMISSION FROM SELECT TARGETS

@article{Siemion2013A1G,
  title={A 1.1–1.9 GHz SETI SURVEY OF THE KEPLER FIELD. I. A SEARCH FOR NARROW-BAND EMISSION FROM SELECT TARGETS},
  author={Andrew P. V. Siemion and Paul B. Demorest and Eric J. Korpela and Ronald J. Maddalena and Dan Werthimer and Jeff Cobb and Andrew W. Howard and Glen I. Langston and Matt Lebofsky and Geoffrey W. Marcy and Jill Tarter},
  journal={The Astrophysical Journal},
  year={2013},
  volume={767}
}
We present a targeted search for narrow-band (<5 Hz) drifting sinusoidal radio emission from 86 stars in the Kepler field hosting confirmed or candidate exoplanets. Radio emission less than 5 Hz in spectral extent is currently known to only arise from artificial sources. The stars searched were chosen based on the properties of their putative exoplanets, including stars hosting candidates with 380 K > Teq > 230 K, stars with five or more detected candidates or stars with a super-Earth (Rp < 3 R… 

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