A Search for Technosignatures Around 31 Sun-like Stars with the Green Bank Telescope at 1.15-1.73 GHz
Jean-Luc Margot, Pavlo Pinchuk, Robert Geil, Stephen Alexander, Sparsh, Arora, Swagata Biswas, Jose Cebreros, Sanjana Prabhu Desai, Benjamin Duclos,, Riley Dunne, Kristy Kwan Lin, Shashwat Goel, Julia Gonzales, Alexander, Gonzalez, Rishabh Jain, Adrian Lam, Briley Lewis

TL;DR
This study used the Green Bank Telescope to search for technosignatures around 31 Sun-like stars at 1.15-1.73 GHz, improving detection methods and analyzing millions of signals, but found no confirmed extraterrestrial signals.
Contribution
The paper introduces an enhanced data processing pipeline with better candidate detection and RFI filtering, increasing detection efficiency in technosignature searches.
Findings
93% signal recovery rate in tests
99.73% of recovered signals identified as candidates
4539 signals outside known RFI regions
Abstract
We conducted a search for technosignatures in April of 2018 and 2019 with the L-band receiver (1.15-1.73 GHz) of the 100 m diameter Green Bank Telescope. These observations focused on regions surrounding 31 Sun-like stars near the plane of the Galaxy. We present the results of our search for narrowband signals in this data set as well as improvements to our data processing pipeline. Specifically, we applied an improved candidate signal detection procedure that relies on the topographic prominence of the signal power, which nearly doubles the signal detection count of some previously analyzed data sets. We also improved the direction-of-origin filters that remove most radio frequency interference (RFI) to ensure that they uniquely link signals observed in separate scans. We performed a preliminary signal injection and recovery analysis to test the performance of our pipeline. We found…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Superconducting and THz Device Technology · Astronomy and Astrophysical Research
