A Search for Brief Optical Flashes Associated with the SETI Target KIC 846285
Abeysekara et al
The F-type star KIC~8462852 has recently been identified as an exceptional target for SETI (search for extraterrestrial intelligence) observations. We describe an analysis methodology for optical SETI, which we have used to analyse nine hours of serendipitous archival observations of KIC~8462852 made with the VERITAS gamma-ray observatory between 2009 and 2015. No evidence of pulsed optical beacons, above a pulse intensity at the Earth of approximately 1 photon per m^2, is found. We also discuss the potential use of imaging atmospheric Cherenkov telescope arrays in searching for extremely short duration optical transients in general.
Wednesday, February 3, 2016
SETI Search for Optical Flashes From KIC 846285 Turns up Negative
Posted by Will Baird at 4:00 AM
Labels: anomaly, f dwarf, KIC 8462852, optical seti, seti
Subscribe to: Post Comments (Atom)
Post a Comment
Note: Only a member of this blog may post a comment.