Pulsar-aided SETI experimental observations

Details Pulsar-aided SETI experimental observations Pulsar-aided SETI experimental observations

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mala.iafcr....h&link_type=abstract

IAF, International Astronautical Congress, 40th, Malaga, Spain, Oct. 7-13, 1989. 7 p.

Astronomy and Astrophysics

Astronomy

Extraterrestrial Communication, Project Seti, Pulsars, Radio Frequencies, Extrasolar Planets, Radio Communication, Radio Frequency Interference, Search Profiles

Scientific paper

The rotational frequencies of pulsars are used to select preferred radio frequencies for SETI. Pulsar rotational frequencies are converted into SETI frequencies in the 1-10 GHz Galactic radio window. Experimental observations using the frequencies are conducted for target stars closer than 25 parsecs, unknown targets in a globular cluster, and unknown targets in the Galaxy closer than 2.5 kpc. The status of these observations is discussed.

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