| Revision as of 21:57, 23 October 2004 edit217.155.203.105 (talk)No edit summary← Previous edit | Revision as of 15:45, 26 November 2004 edit undoZeroOne (talk | contribs)Extended confirmed users, Pending changes reviewers7,451 editsm megahertzNext edit → | ||
| Line 1: | Line 1: | ||
| {{wrongtitle|title=Radio source SHGb02+14a}} | {{wrongtitle|title=Radio source SHGb02+14a}} | ||
| '''SHGb02+14a''' is an interesting radio source and candidate in the ] discovered by ] and announced in '']'' on ], ]. This weak source was observed three times at 1420 megahertz. There is no star within 1000 ]s of its direction. | '''SHGb02+14a''' is an interesting radio source and candidate in the ] discovered by ] and announced in '']'' on ], ]. This weak source was observed three times at 1420 ]. There is no star within 1000 ]s of its direction. | ||
| A more skeptical article concerning the discovery was written by ]. | A more skeptical article concerning the discovery was written by ]. | ||
Revision as of 15:45, 26 November 2004
The correct title of this article is Radio source SHGb02+14a. It appears incorrectly here due to technical restrictions.SHGb02+14a is an interesting radio source and candidate in the Search for Extra-Terrestrial Intelligence discovered by SETI@home and announced in New Scientist on September 1, 2004. This weak source was observed three times at 1420 megahertz. There is no star within 1000 light years of its direction. A more skeptical article concerning the discovery was written by The Planetary Society.