TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2358 SUBJECT: GRB 030821(=H2814): A Faint, Long GRB Localized by the HETE WXM and the IPN DATE: 03/08/22 02:02:16 GMT FROM: Don Lamb at U.Chicago T. Donaghy, C. Graziani, Y. Shirasaki, T. Tamagawa, M. Suzuki, M. Matsuoka, K. Torii, T. Sakamoto, A. Yoshida, E. Fenimore, M. Galassi, Y. Nakagawa, R. Satoh, Y. Urata, T. Yamazaki and Y. Yamamoto, 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; G. Prigozhin, N. Butler, G. Crew, J. Doty, A. Dullighan, R. Vanderspek, J. Villasenor, J. G. Jernigan, A. Levine, F. Martel, E. Morgan, G. Monnelly, G. Azzibrouck, J. Braga, R. Manchanda, and G. Pizzichini, on behalf of the HETE Operations and HETE Optical-SXC Teams; C. Barraud, M. Boer, J-F Olive, and J-P Dezalay on behalf of the HETE FREGATE Team; K. Hurley and T. Cline, on behalf of the Ulysses, HETE, Mars Odyssey, and KONUS GRB teams; I. Mitrofanov, S. Charyshnikov, V. Grinkov, A. Kozyrev, M. Litvak, and A. Sanin, on behalf of the HEND-Odyssey GRB team; W. Boynton, C. Fellows, K. Harshman, C. Shinohara and R. Starr, on behalf of the GRS-Odyssey GRB team; E. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team; A. von Kienlin, G. Lichti, and A. Rau, on behalf of the INTEGRAL SPI-ACS GRB team, report: At 05:31:50 UTC (19895.60 s UT) on 21 August 2003, the HETE FREGATE and WXM instruments detected GRB 030821 (=H2814), a faint long GRB. The burst triggered FREGATE in the 25-400 keV energy band. A GCN burst alert was issued 15 s later. The burst was faint and located at the edge of the FOV of the WXM YB counter; hence no WXM flight localization was derived. Ground analysis of the WXM data provided a localization that was reported in a GCN Notice (Seq. 3) at 08:45:53 UT. Mars Odyssey (HEND), Konus-Wind, and INTEGRAL (SPI-ACS) also observed this burst. Triangulation of the burst produces a preliminary annulus centered at RA = 341.285, Dec = -15.283 (J2000), whose radius is 32.642 +/- 1.153 degrees (3 sigma). This annulus does not include the initial (Seq. 3) HETE-2 WXM ground analysis location, but is fully consistent with the revised ground analysis location that was reported in a GCN Notice (Seq. 4) at 22:12:10 UT. The revised WXM ground analysis localization can be expressed as a rectangle that is 33 arcminutes wide and 3.3 degrees long, whose center is at WXM Center-ground: RA = +21h 42m 33s, Dec = -45d 12' 12" (J2000). The four corners of the WXM localization region are located at the following coordinates (J2000): WXM_CORNER1: RA = +21h 41m 48s, Dec = -43d 35' 2" WXM_CORNER2: RA = +21h 45m 58s, Dec = -46d 46' 16" WXM_CORNER3: RA = +21h 43m 16s, Dec = -46d 49' 23" WXM_CORNER4: RA = +21h 39m 10s, Dec = -43d 38' 10" The burst was very faint in the SXC X-camera and was outside the FOV of the SXC Y-camera; hence an SXC localization is unlikely. The T_90 duration of the burst in the 30-400 keV band was ~ 19 s. The peak photon energy flux in 1 s and the fluence of the burst were 4.8 x 10-7 ergs cm-2 s-1 and 5.7 x 10-6 ergs cm-2, respectively, in the same energy band. Ulysses data are expected shortly, and may constrain the localization further. A light curve and finding chart for GRB030821 are provided at the following URL: http://space.mit.edu/HETE/Bursts/GRB030821