About: Radio source SHGb02+14a

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About: Radio source SHGb02+14a Sponge Permalink

An Entity of Type : owl:Thing, within Data Space : dbkwik.org associated with source dataset(s)

Radio source SHGb02+14a is a source and a candidate in the Search for Extra-Terrestrial Intelligence (SETI), discovered on March 2003 by SETI@home and announced in New Scientist on September 1, 2004. The source was observed three times at a frequency of about 1420 MHz, which is expected to be a frequency used by extraterrestrials due to its proximity to one of the main frequencies at which hydrogen absorbs and radiates photons.

Attributes	Values
rdfs:label	Radio source SHGb02+14a
rdfs:comment	Radio source SHGb02+14a is a source and a candidate in the Search for Extra-Terrestrial Intelligence (SETI), discovered on March 2003 by SETI@home and announced in New Scientist on September 1, 2004. The source was observed three times at a frequency of about 1420 MHz, which is expected to be a frequency used by extraterrestrials due to its proximity to one of the main frequencies at which hydrogen absorbs and radiates photons.
sameAs	dbr:Radio_source_SHGb02+14a
dcterms:subject	Mysteries Communication
dbkwik:alienresear...iPageUsesTemplate	dbkwik:resource/7t_qPwUlq6ePVQpOkpYKXQ==
abstract	Radio source SHGb02+14a is a source and a candidate in the Search for Extra-Terrestrial Intelligence (SETI), discovered on March 2003 by SETI@home and announced in New Scientist on September 1, 2004. The source was observed three times at a frequency of about 1420 MHz, which is expected to be a frequency used by extraterrestrials due to its proximity to one of the main frequencies at which hydrogen absorbs and radiates photons.

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