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SETI@home ("SETI at home") is a project of the Berkeley SETI Research Center to analyze radio signals with the aim of searching for signs of extraterrestrial intelligence. Until March 2020, it was run as an Internet-based public volunteer computing project that employed the BOINC software platform.
The SETI@home project used volunteer computing to analyze signals acquired by the SERENDIP project. SETI@home was conceived by David Gedye along with Craig Kasnoff and is a popular volunteer computing project that was launched by the Berkeley SETI Research Center at the University of California, Berkeley, in May 1999.
SETI@home, one of the first and largest public volunteer distributed computing projects, shuts down. It sent millions of chunks of telescope data to computers around the world – ca. 144,000 as of March 2020 – which analyse the radio signals to search for extraterrestrial intelligence (SETI) and send back their results.
The Berkeley SETI Research Center also hosts the Breakthrough Listen program, [4] [5] [6] which is a ten-year initiative with $100 million funding begun in July 2015 to actively search for intelligent extraterrestrial communications in the universe, in a substantially expanded way, using resources that had not previously been extensively used for the purpose.
SETI@home beta, is a hibernating volunteer computing project using the Berkeley Open Infrastructure for Network Computing platform, as a test environment for future SETI@home projects: AstroPulse is a volunteer computing project searching for primordial black holes , pulsars , and ETI .
SHGb02+14a is an astronomical radio source and a candidate in the Search for Extra-Terrestrial Intelligence (SETI), discovered in March 2003 by SETI@home and announced in New Scientist on September 1, 2004. [1]
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Astropulse also makes contributions to the search for ET: first, project proponents believe it may identify a different type of ET signal not identified by the original SETI@Home algorithm; second, proponents believe it may create additional support for SETI by providing a second possible concrete result from the overall search project.