The SERENDIP Project
By Bob Dixon
With Additions By Herb Johnson
SERENDIP Computer System
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SERENDIP Computer
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SERENDIP Display
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In 1995 a new four-million channel spectrum analyzer was
built for us by the folks at the University of California at Berkeley.
Named SERENDIP III, it is the third of a series of SETI receivers previously
moved around the world onto "host" telescopes which were conducting
astrophysical research: hence, a "serendipitous" SETI program. Ours
is the first permanent installation. Our SERENDIP III receiver
increases the sensitivity of the telescope to intelligent, narrow-band,
signals by a factor of 300 over LOBES. It must take turns with the LOBES
program as it requires that the telescope be operated differently from
LOBES. While LOBES switches between the two horn beams 73 times a second to
subtract out local interference, SERENDIP looks at one beam each second.
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Copyright © 1996-2005 Ohio State University Radio Observatory and North American AstroPhysical Observatory.
Originally designed by Point & Click Software, Inc.
Last modified: August 13, 2005
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