------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2206 2006 Mar 03 16.54UT 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 060218 = SUPERNOVA 2006aj N. Gehrels, GSFC, on behalf of the SWIFT team, points out on GCN 4787 that GRB 060218 is a strange event. It has - a gamma-ray light curve that is flat and a soft spectrum - an X-ray light curve with a long, slow rise and gradual decline - an optical light curve with brightening after 10 hours (Marshall et al. GCN 4785). These characteristics are unlike previous GRBs. It has properties that are also atypical of a transient: - it is far off the galactic plane (b = -32.9 deg) and far away from the bulge (l = 166.9 deg) - there is a possible association with a galaxy in the SDSS pre-burst field. A. M. Soderberg, et. al., Caltech reports on GCN 4804 on an optical spectrum of the afterglow with GMOS on the Gemini-south telescope starting on 2006 Feb 21.024 UT. They confirm the presence of narrow emission lines at z=0.033, as well as the presence of broad absorption features similar to those seen in SN1998bw and other broad-lined Type Ibc supernovae. Jan-Erik Ovaldsen reports on GCN 4818 that observations with DFOSC on the Danish 1.5m telescope at La Silla/ESO show the optical afterglow + SN 2006aj has brightened by 0.2 (+/- 0.01) mag in R and 0.1 (+/- 0.02) mag in V from Feb 21.03 UT to Feb 22.03 UT. An optical brightening is in line with the notion that the underlying SN 2006aj has still to reach its maximum, as noted in previous reports. Editor: Following the nomination of this object by Julie Chignell at last Saturday's BAA Workshop in Milton Keynes for possible imaging with the Faulkes Telescope but thwarted by cloud, Nick James reports successfully imaging it on 2006 Feb 28 at 19.01UT. He estimated it at magnitude 17.6 (unfiltered) confirming the brightening. SUPERNOVA 2006ae IN ANONYMOUS GALAXY Discovery by SDSS Collaboration of a possible supernova (IAUC 8674): SN 2005 UT R.A. (2000.0) Decl. Mag. Offset 2006ae Feb. 2.51 14 48 23.27 +21 47 51.5 20.7 Centre SUPERNOVA 2006af IN ANONYMOUS GALAXY Discovery by SDSS Collaboration of a possible supernova (IAUC 8674): SN 2005 UT R.A. (2000.0) Decl. Mag. Offset 2006af Feb. 4.38 10 33 57.18 +20 20 25.7 19.5 Centre SUPERNOVA 2006ag IN ANONYMOUS GALAXY Discovery by the Nearby Supernova factory of a possible supernova (IAUC 8674): SN 2005 UT R.A. (2000.0) Decl. Mag. Offset 2006ag Feb. 9.4 12 00 17.12 +28 36 22.0 17.9 - SUPERNOVA 2006ah IN ANONYMOUS GALAXY Discovery by the Nearby Supernova factory of a possible supernova (IAUC 8674): SN 2005 UT R.A. (2000.0) Decl. Mag. Offset 2006ah Feb. 9.6 13 46 13.71 -09 07 50.6 18.6 - SUPERNOVA 2006ai IN ESO 5-G9 Discovery by Luckas, Trondal and Schwartz of a possible supernova (IAUC 8674): SN 2005 UT R.A. (2000.0) Decl. Mag. Offset 2006ai Feb. 17.54 07 29 52.16 -84 02 20.5 16.2 2.5"W, 1.8"S Guy M Hurst