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Searching the SETI Ellipsoid with Gaia
In developing robust searches for technosignatures—signs of technological activity from extraterrestrial sources—we must confront choices on both the types of signals that will be explored from our data, as well as which stars to observe and when (Tarter 2001). While this is broadly true for all studies in observational astronomy that explore detection limits on rare phenomena, it is especially so in the search for extraterrestrial intelligence (SETI).
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