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The Breakthrough Listen Search for Intelligent Life: A 3.95–8.00 GHz Search for Radio Technosignatures in the Restricted Earth Transit Zone

机译:突破倾听智能生活的搜索:3.95-8.00 GHz搜索受限制的地球传输区的无线电技术

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We report on a search for artificial narrowband signals of 20 stars within the restricted Earth Transit Zone (rETZ) as a part of the ten-year Breakthrough Listen (BL) search for extraterrestrial intelligence (ETI). The rETZ is the region of the sky from which an observer would see Earth transit the Sun with an impact parameter of less than 0.5. This region of the sky is geometrically unique, providing a potential way for an ETI to discover the solar system. The targets were nearby (7–143 pc) and the search covered an electromagnetic frequency range of 3.95–8.00 GHz. We used the Robert C. Byrd Green Bank Telescope to perform these observations with the standard BL data recorder. We searched these data for artificial narrowband (~Hz) signals with Doppler drift rates of ±20 Hz s?1. We find no evidence for radio technosignatures from ETI in our observations. The observing campaign would have allowed for detections of emissions that were 10?3 to 0.88 times as powerful as the signaling capability of the Arecibo radar transmitter. We conclude that at least 0.6% of the systems in the rETZ within 150 pc do not possess the type of transmitters searched in this survey. To our knowledge, this is the first targeted search for ETI of the rETZ. All data used in this paper are publicly available via the BL Public Data Archive (http://seti.berkeley.edu/bldr2).
机译:我们报告了在限制地球传输区(RETZ)内的20颗星的人工窄带信号的搜索,作为十年突破性的一部分(BL)寻找外星智力(ETI)。 RETZ是天空的区域,观察者将看到地球在阳光下的影响,影响参数小于0.5。这个地区的天空是几何唯一的,为ETI提供了一种潜在的方式来发现太阳系。附近的目标(7-143 PC),搜索涵盖了3.95-8.00 GHz的电磁频率范围。我们使用Robert C. Byrd Green Bank望远镜与标准BL数据记录器进行这些观察。我们在人造窄带(〜Hz)信号中搜索了这些数据,其中多普勒漂移率为±20 Hzs≤1。我们发现我们的观察中没有从ETI获取无线电技术的证据。观察活动将允许检测10?3至0.88倍的排放,作为Arexibo雷达发射器的信令能力。我们得出结论,在150台PC中的RETZ中的至少0.6%的系统不具有本调查中搜索的发射机类型。为了我们的知识,这是第一个有针对性的eti的搜索。本文中使用的所有数据都通过BL公共数据存档公开可用(http://seti.berkeley.edu/bldr2)。

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