HETE observations of the gamma-ray burst GRB 030329: Evidence for an underlying soft X-ray component

R. Vanderspek; T. Sakamoto; C. Barraud; T. Tamagawa; C. Graziani; M. Suzuki; Y. Shirasaki; G. Prigozhin; J. Villasenor; J. G. Jernigan; G. B. Crew; J. L. Atteia; K. Hurley; N. Kawai; D. Q. Lamb; G. R. Ricker; S. E. Woosley; N. Butler; J. P. Doty; A. Dullighan; T. Q. Donaghy; E. E. Fenimore; M. Galassi; M. Matsuoka; K. Takagishi; K. Torii; A. Yoshida; M. Boer; J. P. Dezalay; J. F. Olive; J. Braga; R. Manchanda; G. Pizzichini

doi:10.1086/423923

HETE observations of the gamma-ray burst GRB 030329: Evidence for an underlying soft X-ray component

R. Vanderspek
, T. Sakamoto
, C. Barraud
, T. Tamagawa
, C. Graziani
, M. Suzuki
, Y. Shirasaki
, G. Prigozhin
, J. Villasenor
, J. G. Jernigan
, G. B. Crew
, J. L. Atteia
, K. Hurley
, N. Kawai
, D. Q. Lamb
, G. R. Ricker
, S. E. Woosley
, N. Butler
, J. P. Doty
, A. Dullighan

T. Q. Donaghy, E. E. Fenimore, M. Galassi, M. Matsuoka, K. Takagishi, K. Torii, A. Yoshida, M. Boer, J. P. Dezalay, J. F. Olive, J. Braga, R. Manchanda, G. Pizzichini

Research output: Contribution to journal › Article › peer-review

61 Scopus citations

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 ∼10 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 Sγ = 1.2 × 10^-4 ergs cm^-2, making GRB 030329 one of the brightest GRBs ever detected. Communication of a 2́ 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 ∼7×10^-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.

Original language	English (US)
Pages (from-to)	1251-1257
Number of pages	7
Journal	Astrophysical Journal
Volume	617
Issue number	2 I
DOIs	https://doi.org/10.1086/423923
State	Published - Dec 20 2004
Externally published	Yes

Keywords

Gamma rays: bursts
X-rays: individual (GRB 030329)

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/423923

Cite this

Vanderspek, R., Sakamoto, T., Barraud, C., Tamagawa, T., Graziani, C., Suzuki, M., Shirasaki, Y., Prigozhin, G., Villasenor, J., Jernigan, J. G., Crew, G. B., Atteia, J. L., Hurley, K., Kawai, N., Lamb, D. Q., Ricker, G. R., Woosley, S. E., Butler, N., Doty, J. P., ... Pizzichini, G. (2004). HETE observations of the gamma-ray burst GRB 030329: Evidence for an underlying soft X-ray component. Astrophysical Journal, 617(2 I), 1251-1257. https://doi.org/10.1086/423923

Vanderspek, R, Sakamoto, T, Barraud, C, Tamagawa, T, Graziani, C, Suzuki, M, Shirasaki, Y, Prigozhin, G, Villasenor, J, Jernigan, JG, Crew, GB, Atteia, JL, Hurley, K, Kawai, N, Lamb, DQ, Ricker, GR, Woosley, SE, Butler, N, Doty, JP, Dullighan, A, Donaghy, TQ, Fenimore, EE, Galassi, M, Matsuoka, M, Takagishi, K, Torii, K, Yoshida, A, Boer, M, Dezalay, JP, Olive, JF, Braga, J, Manchanda, R & Pizzichini, G 2004, 'HETE observations of the gamma-ray burst GRB 030329: Evidence for an underlying soft X-ray component', Astrophysical Journal, vol. 617, no. 2 I, pp. 1251-1257. https://doi.org/10.1086/423923

@article{8726c5a40baf48c8a29678b95630688e,

title = "HETE observations of the gamma-ray burst GRB 030329: Evidence for an underlying soft X-ray component",

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 ∼10 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 Sγ = 1.2 {\texttimes} 10-4 ergs cm-2, making GRB 030329 one of the brightest GRBs ever detected. Communication of a {\'2} 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 ∼7{\texttimes}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.",

keywords = "Gamma rays: bursts, X-rays: individual (GRB 030329)",

author = "R. Vanderspek and T. Sakamoto and C. Barraud and T. Tamagawa and C. Graziani and M. Suzuki and Y. Shirasaki and G. Prigozhin and J. Villasenor and Jernigan, \{J. G.\} and Crew, \{G. B.\} and Atteia, \{J. L.\} and K. Hurley and N. Kawai and Lamb, \{D. Q.\} and Ricker, \{G. R.\} and Woosley, \{S. E.\} and N. Butler and Doty, \{J. P.\} and A. Dullighan and Donaghy, \{T. Q.\} and Fenimore, \{E. E.\} and M. Galassi and M. Matsuoka and K. Takagishi and K. Torii and A. Yoshida and M. Boer and Dezalay, \{J. P.\} and Olive, \{J. F.\} and J. Braga and R. Manchanda and G. Pizzichini",

year = "2004",

month = dec,

day = "20",

doi = "10.1086/423923",

language = "English (US)",

volume = "617",

pages = "1251--1257",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2 I",

}

TY - JOUR

T1 - HETE observations of the gamma-ray burst GRB 030329

T2 - Evidence for an underlying soft X-ray component

AU - Vanderspek, R.

AU - Sakamoto, T.

AU - Barraud, C.

AU - Tamagawa, T.

AU - Graziani, C.

AU - Suzuki, M.

AU - Shirasaki, Y.

AU - Prigozhin, G.

AU - Villasenor, J.

AU - Jernigan, J. G.

AU - Crew, G. B.

AU - Atteia, J. L.

AU - Hurley, K.

AU - Kawai, N.

AU - Lamb, D. Q.

AU - Ricker, G. R.

AU - Woosley, S. E.

AU - Butler, N.

AU - Doty, J. P.

AU - Dullighan, A.

AU - Donaghy, T. Q.

AU - Fenimore, E. E.

AU - Galassi, M.

AU - Matsuoka, M.

AU - Takagishi, K.

AU - Torii, K.

AU - Yoshida, A.

AU - Boer, M.

AU - Dezalay, J. P.

AU - Olive, J. F.

AU - Braga, J.

AU - Manchanda, R.

AU - Pizzichini, G.

PY - 2004/12/20

Y1 - 2004/12/20

N2 - 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 ∼10 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 Sγ = 1.2 × 10-4 ergs cm-2, making GRB 030329 one of the brightest GRBs ever detected. Communication of a 2́ 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 ∼7×10-6 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.

AB - 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 ∼10 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 Sγ = 1.2 × 10-4 ergs cm-2, making GRB 030329 one of the brightest GRBs ever detected. Communication of a 2́ 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 ∼7×10-6 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.

KW - Gamma rays: bursts

KW - X-rays: individual (GRB 030329)

UR - https://www.scopus.com/pages/publications/13944269199

UR - https://www.scopus.com/pages/publications/13944269199#tab=citedBy

U2 - 10.1086/423923

DO - 10.1086/423923

M3 - Article

AN - SCOPUS:13944269199

SN - 0004-637X

VL - 617

SP - 1251

EP - 1257

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 I

ER -

HETE observations of the gamma-ray burst GRB 030329: Evidence for an underlying soft X-ray component

Abstract

Keywords

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