# The Breakthrough Listen Search for Intelligent Life: Observations of   1327 Nearby Stars over 1.10-3.45 GHz

**Authors:** Danny C. Price, J. Emilio Enriquez, Bryan Brzycki, Steve Croft, Daniel, Czech, David DeBoer, Julia DeMarines, Griffin Foster, Vishal Gajjar, Nectaria, Gizani, Greg Hellbourg, Howard Isaacson, Brian Lacki, Matt Lebofsky, David H., E. MacMahon, Imke de Pater, Andrew P. V. Siemion, Dan Werthimer, James A., Green, Jane F. Kaczmarek, Ronald J. Maddalena, Stacy Mader, Jamie Drew, and, S. Pete Worden

arXiv: 1906.07750 · 2020-02-07

## TL;DR

This paper reports on a comprehensive radio survey of 1327 nearby stars using the Green Bank and Parkes telescopes, searching for technosignatures in the 1.10-3.45 GHz range, with no candidates found, setting upper limits on transmitter power.

## Contribution

It presents the most extensive search for extraterrestrial technosignatures in the 1.10-3.45 GHz range, detailing data analysis techniques and providing a large dataset for future research.

## Key findings

- No technosignature candidates detected.
- Set upper limits on potential transmitter power.
- Produced and released 219 TB of observational data.

## Abstract

Breakthrough Listen (BL) is a ten-year initiative to search for signatures of technologically capable life beyond Earth via radio and optical observations of the local Universe. A core part of the BL program is a comprehensive survey of 1702 nearby stars at radio wavelengths (1-10 GHz). Here, we report on observations with the 64-m CSIRO Parkes radio telescope in New South Wales, Australia, and the 100-m Robert C. Byrd Green Bank radio telescope in West Virginia, USA. Over 2016 January to 2019 March, a sample of 1138 stars was observed at Green Bank using the 1.10-1.90 GHz and 1.80-2.80 GHz receivers, and 189 stars were observed with Parkes over 2.60-3.45 GHz. We searched these data for the presence of engineered signals with Doppler-acceleration drift rates between -4 to 4 Hz/s. Here, we detail our data analysis techniques and provide examples of detected events. After excluding events with characteristics consistent with terrestrial radio interference, we are left with zero candidates. Given the sensitivity of our observations, we can put an upper limit on the power of potential radio transmitters at these frequencies at 2x10^12 W, and 9x10^12 W for GBT and Parkes respectively. These observations constitute the most comprehensive search over 1.10-3.45 GHz for technosignatures to date. All data products, totalling ~219 TB, are available for download as part of the first BL data release (DR1), as described in a companion paper (Lebofsky et. al., 2019)

## Full text

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## Figures

30 figures with captions in the complete paper: https://tomesphere.com/paper/1906.07750/full.md

## References

74 references — full list in the complete paper: https://tomesphere.com/paper/1906.07750/full.md

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Source: https://tomesphere.com/paper/1906.07750