A 1.1 to 1.9 GHz SETI Survey of the Kepler Field: I. A Search for Narrow-band Emission from Select Targets
Andrew P. V. Siemion, Paul Demorest, Eric Korpela, Ron J. Maddalena,, Dan Werthimer, Jeff Cobb, Andrew W. Howard, Glen Langston, Matt Lebofsky,, Geoffrey W. Marcy, Jill Tarter

TL;DR
This paper reports a targeted search for narrow-band radio signals from 86 Kepler stars with exoplanets, finding no extraterrestrial signals and setting upper limits on the prevalence of radio-loud civilizations in the galaxy.
Contribution
The study conducted a comprehensive search for narrow-band extraterrestrial signals from specific Kepler stars, establishing new upper limits on the abundance of radio-loud civilizations.
Findings
No extraterrestrial narrow-band signals detected.
Fewer than 1% of transiting exoplanet systems host detectable radio civilizations.
Limits on the number of Kardashev type II civilizations in the Milky Way.
Abstract
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 > T_eq > 230 K, stars with 5 or more detected candidates or stars with a super-Earth (R_p < 3 R_earth) in a > 50 day orbit. Baseband voltage data across the entire band between 1.1 and 1.9 GHz were recorded at the Robert C. Byrd Green Bank Telescope between Feb--Apr 2011 and subsequently searched offline. No signals of extraterrestrial origin were found. We estimate that fewer than ~1% of transiting exoplanet systems host technological civilizations that are radio loud in narrow-band…
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