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arXiv · 2006.13789

Breakthrough Listen Search for Technosignatures Towards the Kepler-160 System

Karen Perez·Bryan Brzycki·Vishal Gajjar·Howard Isaacson·Andrew Siemion·Steve Croft·David DeBoer·Matt Lebofsky·David H. E. MacMahon·Danny C. Price·Sofia Sheikh·Jamie Drew·S. Pete Worden
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Abstract

We have conducted a search for artificial radio emission associated with the Kepler-160 system following the report of the discovery of the Earth-like planet candidate KOI-456.04 on 2020 June 4 (arXiv:1905.09038v2). Our search targeted both narrowband (2.97 Hz) drifting ($\pm 4$ Hz s$^{-1})$ and wideband pulsed (5 ms at all bandwidths) artificially-dispersed technosignatures using the turboSETI (arXiv:1709.03491v2) and SPANDAK pipelines, respectively, from 1-8 GHz. No candidates were identified above an upper limit Equivalent Isotropic Radiated Power (EIRP) of $5.9 \times 10^{14}$ W for narrowband emission and $7.3 \times 10^{12}$ W for wideband emission. Here we briefly describe our observations and data reduction procedure.

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Karen Perez, Bryan Brzycki, Vishal Gajjar, Howard Isaacson, Andrew Siemion, Steve Croft, David DeBoer, Matt Lebofsky, David H. E. MacMahon, Danny C. Price, Sofia Sheikh, Jamie Drew, S. Pete Worden. 2020-06-22. Breakthrough Listen Search for Technosignatures Towards the Kepler-160 System. https://arxiv.org/abs/2006.13789

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