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Woosley, T. Cline, T. Q. Donaghy, T. Sakamoto, T. Tamagawa, Y. Shirasaki","submitted_at":"2003-03-20T16:53:55Z","abstract_excerpt":"A bright, x-ray-rich GRB was detected by HETE-2 at 11:18:34.03 UT on 11 Dec 2002. The WXM localization was to 14' and relayed to the GCN 22 s after the start of the burst. The ground SXC localization was within 2' of R.A. 08h 09m 00s, Dec 06d 44' 20\" (J2000). GRB021211 consists of a single, FRED-like pulse with t90s of 2.3 s (85-400 keV) and 8.5 s (2-10 keV). The peak photon number and photon energy fluxes in the 2-400 keV band, are 34.0 +/- 1.8 ph cm^-2 s^-1 and 1.68 +/- 0.11 x 10^-6 erg cm^-2 s^-1, respectively. 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Levine, A. Yoshida, C. Barraud, C. Graziani, D. Q. Lamb, E. E. Fenimore, E. Morgan, F. Martel, G. B. Crew, G. Monnelly, G. Pizzichini, G. Prigozhin, G. R. Ricker, J. Braga, J. Doty, J.-F. Olive, J. G. Jernigan, J.-L. Atteia, J.-P. Dezalay, J. Villasenor, K. Hurley, K. Takagishi, K. Torii, M. Boer, M. Galassi, M. Matsuoka, M. Suzuki, M. Yamauchi, N. Butler, N. Kawai, R. Manchanda, R. Vanderspek, S. E. Woosley, T. Cline, T. Q. Donaghy, T. Sakamoto, T. Tamagawa, Y. Shirasaki","submitted_at":"2003-03-20T16:53:55Z","abstract_excerpt":"A bright, x-ray-rich GRB was detected by HETE-2 at 11:18:34.03 UT on 11 Dec 2002. The WXM localization was to 14' and relayed to the GCN 22 s after the start of the burst. The ground SXC localization was within 2' of R.A. 08h 09m 00s, Dec 06d 44' 20\" (J2000). GRB021211 consists of a single, FRED-like pulse with t90s of 2.3 s (85-400 keV) and 8.5 s (2-10 keV). 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