New SETI Sky Surveys for Radio Pulses
Andrew Siemion (1,4), Joshua Von Korff (3), Peter McMahon (4,5), Eric, Korpela (2), Dan Werthimer (2,4), David Anderson (2), Geoff Bower (1), Jeff, Cobb (2), Griffin Foster (1), Matt Lebofsky (2), Joeri van Leeuwen (1), Mark, Wagner (4) ((1) Astronomy Department

TL;DR
This paper reviews two new SETI sky survey efforts, Astropulse and Fly's Eye, which aim to detect microsecond to millisecond radio pulses from various potential sources, including extraterrestrial civilizations.
Contribution
It introduces two orthogonal radio pulse search programs with unprecedented sensitivity and sky coverage, utilizing innovative data analysis and volunteer computing techniques.
Findings
Detected three pulsars and six giant pulses from Crab pulsar
Astropulse is 30 times more sensitive than previous searches
Approximately 450 hours of Fly's Eye observations conducted
Abstract
Berkeley conducts 7 SETI programs at IR, visible and radio wavelengths. Here we review two of the newest efforts, Astropulse and Fly's Eye. A variety of possible sources of microsecond to millisecond radio pulses have been suggested in the last several decades, among them such exotic events as evaporating primordial black holes, hyper-flares from neutron stars, emissions from cosmic strings or perhaps extraterrestrial civilizations, but to-date few searches have been conducted capable of detecting them. We are carrying out two searches in hopes of finding and characterizing these mu-s to ms time scale dispersed radio pulses. These two observing programs are orthogonal in search space; the Allen Telescope Array's (ATA) "Fly's Eye" experiment observes a 100 square degree field by pointing each 6m ATA antenna in a different direction; by contrast, the Astropulse sky survey at Arecibo…
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