Talk:Rotating radio transient

A fact from Rotating radio transient appeared on Wikipedia's Main Page in the Did you know column on 1 December 2009 (check views). The text of the entry was as follows:

Did you know... that rotating radio transients are among the brightest astronomical sources of radio waves, yet are generally detectable for less than one second a day?

A record of the entry may be seen at Wikipedia:Recent additions/2009/December.

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Merge from Rotating radio transients[edit]

Noticing a very old merge tag on the page (this revision; tagged since September), I merged the two. Rotating radio transients was largely a duplicate article, even citing one of the same sources. Fortunately, both are small enough so that merging consists of adding a source and changing one into a redirect. Ourai ^т _с 02:48, 5 December 2006 (UTC)[reply]

Should we list or tabulate some notable ones[edit]

Maybe none are notable (apart from RRAT J1819-1458) ? - Rod57 (talk) 08:58, 29 April 2015 (UTC)[reply]