The Breakthrough Listen Search for Intelligent Life: 1.1-1.9GHz Observations of 692 Nearby Stars

被引:78
作者
Enriquez, J. Emilio [1 ,2 ]
Siemion, Andrew [1 ,2 ,3 ]
Foster, Griffin [1 ,4 ]
Gajjar, Vishal [5 ]
Hellbourg, Greg [1 ]
Hickish, Jack [6 ]
Isaacson, Howard [1 ]
Price, Danny C. [1 ,7 ]
Croft, Steve [1 ]
DeBoer, David [6 ]
Lebofsky, Matt [1 ]
MacMahon, David H. E. [6 ]
Werthimer, Dan [1 ,5 ,6 ]
机构
[1] Univ Calif Berkeley, Dept Astron, 501 Campbell Hall 3411, Berkeley, CA 94720 USA
[2] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands
[3] SETI Inst, Mountain View, CA 94043 USA
[4] Univ Oxford, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
[5] Univ Calif Berkeley, Space Sci Lab, 7 Gauss way, Berkeley, CA 94720 USA
[6] Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA
[7] Swinburne Univ Technol, Ctr Astrophys & Supercomp, POB 218, Hawthorn, Vic 3122, Australia
关键词
astrobiology; extraterrestrial intelligence; EXTRATERRESTRIAL INTELLIGENCE; SETI OBSERVATIONS; TARGET SELECTION; PROJECT PHOENIX; SIGNALS; POSITRONIUM; EXOPLANETS; TELESCOPE; FREQUENCY; SERENDIP;
D O I
10.3847/1538-4357/aa8d1b
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on a search for engineered signals from a sample of 692 nearby stars using the Robert C. Byrd Green Bank Telescope, undertaken as part of the Breakthrough Listen Initiative search for extraterrestrial intelligence. Observations were made over 1.1-1.9 GHz (L band), with three sets of five-minute observations of the 692 primary targets, interspersed with five-minute observations of secondary targets. By comparing the "ON" and "OFF" observations, we are able to identify terrestrial interference and place limits on the presence of engineered signals from putative extraterrestrial civilizations inhabiting the environs of the target stars. During the analysis, 11 events passed our thresholding algorithm, but a detailed analysis of their properties indicates that they are consistent with known examples of anthropogenic radio-frequency interference. We conclude that, at the time of our observations, none of the observed systems host high-duty-cycle radio transmitters emitting between 1.1 and 1.9 GHz with an Equivalent Isotropic Radiated Power of similar to 10(13) W, which is readily achievable by our own civilization. Our results suggest that fewer than similar to 0.1% of the stellar systems within 50 pc possess the type of transmitters searched in this survey.
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页数:13
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