Please use this identifier to cite or link to this item: https://www.um.edu.mt/library/oar/handle/123456789/146099
Title: The breakthrough listen search for intelligent life : technosignature search of 97 nearby galaxies
Authors: Choza, Carmen
Bautista, Daniel
Croft, Steve
Siemion, Andrew P. V.
Brzycki, Bryan
Bhattaram, Krishnakumar
Czech, Daniel
de Pater, Imke
Gajjar, Vishal
Isaacson, Howard
Lacker, Kevin
Lacki, Brian
Lebofsky, Matthew
MacMahon, David H. E.
Price, Danny
Schoultz, Sarah
Sheikh, Sofia
Varghese, Savin Shynu
Morgan, Lawrence
Drew, Jamie
Worden, S. Pete
Keywords: Extraterrestrial beings -- Research
Life on other planets
Radio astronomy
Galaxies -- Observations
Signal processing -- Digital techniques
Issue Date: 2024
Publisher: IOPscience
Citation: Choza, C., Bautista, D., Croft, S., Siemion, A. P., Brzycki, B., Bhattaram, K.,...Worden, S. P. (2024). The breakthrough listen search for Intelligent Life: Technosignature search of 97 nearby galaxies. The Astronomical Journal, 167(1), 10.
Abstract: The Breakthrough Listen search for intelligent life is, to date, the most extensive technosignature search of nearby celestial objects. We present a radio technosignature search of the centers of 97 nearby galaxies, observed by Breakthrough Listen at the Robert C. Byrd Green Bank Telescope. We performed a narrowband Doppler drift search using the turboSETI pipeline with a minimum signal-to-noise parameter threshold of 10, across a drift rate range of ±4 Hz s−1, with a spectral resolution of 3 Hz and a time resolution of ∼18.25 s. We removed radio frequency interference (RFI) by using an on-source/off-source cadence pattern of six observations and discarding signals with Doppler drift rates of 0. We assess factors affecting the sensitivity of the Breakthrough Listen data reduction and search pipeline using signal injection and recovery techniques and apply new methods for the investigation of the RFI environment. We present results in four frequency bands covering 1–11 GHz, and place constraints on the presence of transmitters with equivalent isotropic radiated power on the order of 1026 W, corresponding to the theoretical power consumption of Kardashev Type II civilizations.
URI: https://www.um.edu.mt/library/oar/handle/123456789/146099
Appears in Collections:Scholarly Works - InsSSA



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