  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.

Earth and Planetary Astrophysics;Instrumentation and Methods for Astrophysics