@Article{VanderspekSBTGSSPVJCAHKLRWBDDDFGMTTYBDOBMP:2004:EvUnSo,
               author = "Vanderspek, R. and Sakamoto, T. and Barraud, C. and Tamagawa, T. 
                         and Graziani, C. and Suzuki, M. and Shirasaki, Y. and Prigozhin, 
                         G. and Villasenor, J. and Jernigan, J. G. and Crew, G. B. and 
                         Atteia, J. L. and Hurley, K. and Kawai, N. and Lamb, D. Q. and 
                         Ricker, G. R. and Woosley, S. E. and Butler, N. and Doty, J. P. 
                         and Dullighan, A. and Donaghy, T. Q. and Fenimore, E. E. and 
                         Galassi, M. and Matsuoka, M. and Takagishi, K. and Torii, K. and 
                         Yoshida, A. and Boer, M. and Dezalay, J. P. and Olive, J. F. and 
                         Braga, Jo{\~a}o and Manchanda, R. and Pizzichini, G.",
          affiliation = "MIT, Ctr Space Res, Cambridge and Tokyo Inst Technol, Dept Phys, 
                         Meguro Ku, Tokyo and RIKEN, Inst Phys \& Chem Res, Wako, Saitama 
                         and Los Alamos Natl Lab, Los Alamos, NM 87545 USA and Observ Midi 
                         Pyrenees, Astrophys Lab, Toulouse, F-31400 France and Univ 
                         Chicago, Dept Astron \& Astrophys, Chicago, IL 60637 USA and Natl 
                         Astron Observ, Tokyo, 1818588 Japan and Univ Calif Berkeley, Space 
                         Sci Lab, Berkeley, CA 94720 USA and Univ Calif Santa Cruz, Dept 
                         Astron \& Astrophys, Santa Cruz, CA 95064 USA and Natl Space Dev 
                         Agcy Japan, Tsukuba Space Ctr, Tsukuba, Ibaraki 3058505 Japan and 
                         Miyazaki Univ, Fac Engn, Miyazaki, 8892192 Japan and Osaka Univ, 
                         Grad Sch Sci, Dept Earth \& Space Sci, Osaka, 5600043 Japan and 
                         Aoyama Gakuin Univ, Dept Phys, Setagaya Ku, Tokyo, 1578572 Japan 
                         and Observ Midi Pyrenees, Ctr Etud Spatiale Rayonnements, 
                         Toulouse, F-31028 4 France and Instituto Nacional de Pesquisas 
                         Espaciais, Dire{\c{c}}{\~a}o(INPE,Dire{\c{c}}{\~a}o) and Tata 
                         Inst Fundamental Res, Dept Astron \& Astrophys, Bombay, 
                         Maharashtra 400005 India and CNR, IASF, Sez Bologna, Bologna, 
                         I-40129 Italy",
                title = "HETE observations of the gamma-ray burst GRB 030329: Evidence for 
                         an underlying soft X-ray component",
              journal = "Astrophysical Journal",
                 year = "2004",
               volume = "617",
               number = "2",
                pages = "1251--1257 Part 1",
                month = "Dec.",
             abstract = "An exceptionally intense gamma-ray burst, GRB 030329, was detected 
                         and localized by the instruments on board the High Energy 
                         Transient Explorer satellite (HETE) at 11: 37: 14 UT on 2003 March 
                         29. The burst consisted of two similar to10 s pulses of roughly 
                         equal brightness and an X-ray tail lasting more than 100 s. The 
                         energy fluence in the 30-400 keV energy band was S-gamma 1.2 x 
                         10(-4) ergs cm(-2), making GRB 030329 one of the brightest GRBs 
                         ever detected. Communication of a 20 error box 73 minutes after 
                         the burst allowed the rapid detection of a counterpart in the 
                         optical, X-ray, and radio and the ensuing discovery of a supernova 
                         with most unusual characteristics. Analyses of the burst light 
                         curves reveal the presence of a distinct, bright, soft X-ray 
                         component underlying the main GRB; the 2-10 keV fluence of this 
                         component is similar to7 x 10(-6) ergs cm(-2). The main pulses of 
                         GRB 030329 were preceded by two soft, faint, nonthermal bumps. We 
                         present details of the HETE observations of GRB 030329.",
           copyholder = "SID/SCD",
                 issn = "0004-637X and 1538-4357",
             language = "en",
           targetfile = "hete, vanderspek.pdf",
        urlaccessdate = "05 maio 2024"
}