A Search for Ultra-Narrowband Signals of Extraterrestrial Origin
PAUL HOROWITZ 1
1 Lyman Laboratory of Physics, Harvard University, Cambridge, Massachusetts 02138
Nearly 200 nearby stars similar to the sun were observed at the 21-centimeter neutral hydrogen wavelength (in the heliocentric frame) with a bandwidth of 1 kilohertz and a resolution of 0.015 hertz, using the Arecibo 305-meter antenna. At this resolution the effects of terrestrial interference are so slight that the detection limit of 4 x 1027 watt per square meter was set by receiver noise alone. No evidence of artificial signals was found.
Submitted on April 10, 1978
Revised on May 26, 1978