TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1956 SUBJECT: GRB030323 (=H2640): A Faint, Long GRB Localized by the HETE WXM and SXC DATE: 03/03/25 21:33:01 GMT FROM: Don Lamb at U.Chicago C. Graziani, Y. Shirasaki, M. Matsuoka, T. Tamagawa, K. Torii, T. Sakamoto, M. Suzuki, A. Yoshida, E. Fenimore, M. Galassi, T. Tavenner, T. Donaghy, Y. Nakagawa, D. Takahashi, R. Satoh, and Y. Urata, on behalf of the HETE WXM Team; G. Ricker, J-L Atteia, N. Kawai, D. Lamb, and S. Woosley on behalf of the HETE Science Team; R. Vanderspek, J. Villasenor, G. Crew, J. Doty, G. Monnelly, N. Butler, T. Cline, J.G. Jernigan, A. Levine, F. Martel, E. Morgan, G. Prigozhin, G. Azzibrouck, J. Braga, R. Manchanda, and G. Pizzichini, on behalf of the HETE Operations and HETE Optical-SXC Teams; M. Boer, J-F Olive, J-P Dezalay, C. Barraud and K. Hurley on behalf of the HETE FREGATE Team; write: At 21:56:57.60 UTC (79017.60 s UT) on 23 Mar 2003, the HETE FREGATE, WXM, and SXC instruments detected event H2460, a faint, long GRB. Ground analysis of the WXM data produced a localization which was reported in a GCN Notice at 02:55:11 UT on 24 Mar, about 5 hours after the burst. The WXM localization SNR was 6. The WXM localization can be expressed as a 90% confidence circle that is 18 arcminutes in radius and is centered at WXM: RA = +11h 06m 54s, Dec = -21d 51' 00" (J2000). Ground analysis of the SXC data for the burst produced a more accurate location which was reported in a GCN Notice at 05:28:51 UT on 24 Mar, about 7 1/2 hours after the burst. The SXC localization can be expressed as a 90% confidence trapezoid, whose base and top are 24.5 and 11 arcminutes, whose height is 4 arcminutes, and whose area is 71 square arcminutes. The center of the trapezoid lies at RA = +11h 06m 06s, Dec = -21d 54' 20" (J2000), and its corners lie at RA = +11h 05m 59.0s, Dec = -21d 48' 43" RA = +11h 05m 56.6s, Dec = -21d 59' 46" RA = +11h 06m 12.5s, Dec = -22d 06' 43" RA = +11h 06m 17.8s, Dec = -21d 42" 11" (J2000). The SXC localization is trapezoidal because its sides are defined by the WXM error circle. The t_90 duration of the burst in the 30-400 keV band was 26 s. The fluence of the burst was 1.1 x 10-6 ergs cm-2 and the peak flux in 1.2 sec was ~1.2 x 10-9 ergs cm-2 s-1 (i.e., ~ 0.05 x Crab flux) in the same energy band. A light curve and skymap for GRB030323 is provided at the following URL: http://space.mit.edu/HETE/Bursts/GRB030323