NASA NTRS · 19900026604
Pulsar-aided SETI experimental observations
Abstract
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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Heidmann, J., Biraud, F., Tarter, J.. 1989-10-01. Pulsar-aided SETI experimental observations. https://ntrs.nasa.gov/citations/19900026604
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