------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2281 2006 Nov 21 16.05UT Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke, Hants, RG22 4PP,England.Telephone/FAX(01256)471074Int:+441256471074 INTERNET: GUY@TAHQ.DEMON.CO.UK Backup: gmh@wdcc1.bnsc.rl.ac.uk WORLD WIDE WEB http://www.theastronomer.org ------------------------------------------------------------------- GRB 061121: BRIGHT OPTICAL COUNTERPART Scott Barthelmy, NASA/GSFC reports on GCN 5823, just issued, that at 15:22:29 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 061121 (trigger=239899). Swift slewed immediately to the burst. The BAT on-board calculated location is RA,Dec 147.252, -13.183 {RA 09h 49m 00s, DEC -13d 10' 57"} (J2000) with an uncertainty of 3 arcmin. The BAT light curve shows an initial pulse of ~3000 cnts/sec lasting ~10 sec. Then a second much brighter peak starts at ~T+50 sec, peaking at T+70 sec (at 32,000 cnts/sec), and ending at ~T+80 sec. The XRT began observing the field at 15:23:24 UT, 55 seconds after the BAT trigger. XRT found a very bright, fading, uncatalogued X-ray source, located at RA(J2000) = 09h 48m 54.5s, Dec(J2000) = -13d 11' 46.4" with an estimated uncertainty of 4.7 arcseconds (90% confidence radius). Sarah Yost of the University of Michigan has reported on the optical counterpart in GCN 5824 received 24 minutes ago: ROTSE-IIIa, located at Siding Spring Observatory, Australia, responded to GRB 061121 (Swift trigger 239899). The first image was at 15:22:49.6 UT, 20.6 s after the burst (7.6 s after the GCN notice time). The unfiltered images are calibrated relative to USNO A2.0. We detect a 14.9 magnitude, fading source with coordinates: RA 09:48:54.4 DEC -13:11:42.2 (2000), with positional uncertainty of 1" or better. A jpeg image is available at: http://www.rotse.net/images/gsb239899_3a02_img.jpg Note that the object marked 65 is the candidate in question. Editor: Further observations would be welcomed from our International Team of observers bearing in mind such sources often fade very rapidly. Guy M Hurst