Talk:Rotating radio transient

The contents of Rotating radio transients was merged into Rotating radio transient. The former page's history now serves to provide attribution for that content in the latter page, and it must not be deleted as long as the latter page exists. For the discussion at that location, see its talk page.

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

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

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