A Search for Optical Laser Emission Using Keck HIRES

摘要

We present a search for laser emissions coming from point sources in the vicinity of 2796 stars, including 1368 Kepler objects-of-interest (KOIs) that host one or more exoplanets. We search for extremely narrow emission lines in the wavelength region between 3640 and 7890 using the Keck 10m telescope and spectroscopy with high-resolution (/=60,000). Laser-emission lines coming from nonnatural sources are distinguished from natural astrophysical sources by being monochromatic and coming from an unresolved point in space. We search for laser emissions located 2-7 from the 2796 target stars. The detectability of laser emissions is limited by Poisson statistics of the photons and scattered light, yielding a detection threshold flux of approximate to 1photonsm(-2)min(-1) for typical Kepler stars and approximate to 100photonsm(-2)min(-1) for solar-type stars within 100lt-yr. Diffraction-limited lasers having a 10m aperture can be detected from 100lt-yr away if their power exceeds 90W, and from 1000lt-yr away (Kepler planets), if their power exceeds 1kW (from lasers located 60-200AU, and 2000-7000AU from the nearby and Kepler stars, respectively). We did not find any such laser emission coming from any of the 2796 target stars. We discuss the implications for the search for extraterrestrial intelligence (SETI).