Observers
Von Korff J.
Siemion A.
KORPELA E.
WERTHIMER D.
McMahon P.
Cobb J.
Lebofsky M.
ANDERSON D.
Bankay B.
Bower G.
Foster G.
van Leeuwen J.
Mallard W.
Wagner M.
Astropulse,
Link
Reference
Von Korff, J., Siemion, A., Korpela, E., Werthimer, D., McMahon, P., Cobb, J., Lebofsky, M., Aanderson, D., Bankay, B., Bower, G., Foster, G., Van Leeuwen, J., Mallard, W., Wagner, M., "New SETI Sky Surverys for Radio Pulses" eprint arXiv:0811.3046 (2008).
Sources for the pulses may include black holes, neutron stars, cosmic strings, or ETI. Data from the 7 beam ALFA receiver at Arecibo is reduced by a distributed computing application that uses a coherent de-dispersion technique to look for short broad-pulses. The multibeam data is sent over the internet to the computers of millions of volunteers to be analyzed.