Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2

T. Sakamoto, D. Q. Lamb, N. Kawai, A. Yoshida, C. Graziani, E. E. Fenimore, T. Q. Donaghy, M. Matsuoka, M. Suzuki, G. Ricker, J. L. Atteia, Y. Shirasaki, T. Tamagawa, K. Torii, M. Galassi, J. Doty, R. Vanderspek, G. B. Crew, J. Villasenor, Nathaniel Butler & 18 others G. Prigozhin, J. G. Jernigan, C. Barraud, M. Boer, J. P. Dezalay, J. F. Olive, K. Hurley, A. Levine, G. Monnelly, F. Martel, E. Morgan, S. E. Woosley, T. Cline, J. Braga, R. Manchanda, G. Pizzichini, K. Takagishi, M. Yamauchi

Research output: Contribution to journalArticle

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Abstract

We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first 3 years of its mission, focusing on the properties of X-ray flashes (XRFs) and X-ray-rich GRBs (XRRs). We find that the numbers of XRFs, XRRs, and GRBs are comparable, and that the durations and the sky distributions of XRFs and XRRs are similar to those of GRBs. We also find that the spectral properties of XRFs and XRRs are similar to those of GRBs, except that the values of the peak energy Epeak obs of the burst spectrum in vFv, the peak energy flux Fpeak, and the energy fluence SE of XRFs are much smaller (and those of XRRs are smaller) than those of GRBs. Finally, we find that the distributions of all three kinds of bursts form a continuum in the [SE(2-30 keV), S E(30-400) keV] plane, the [SE(2-400 keV), E peak] plane, and the [Fpeak(50-300 keV), E peak] plane. These results provide strong evidence that all three kinds of bursts arise from the same phenomenon.

Original languageEnglish (US)
Pages (from-to)311-327
Number of pages17
JournalAstrophysical Journal
Volume629
Issue number1 I
DOIs
StatePublished - Aug 10 2005
Externally publishedYes

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gamma ray bursts
flash
x rays
bursts
energy flux
energy
sky
fluence
continuums

Keywords

  • Gamma rays: bursts

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Sakamoto, T., Lamb, D. Q., Kawai, N., Yoshida, A., Graziani, C., Fenimore, E. E., ... Yamauchi, M. (2005). Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2. Astrophysical Journal, 629(1 I), 311-327. https://doi.org/10.1086/431235

Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2. / Sakamoto, T.; Lamb, D. Q.; Kawai, N.; Yoshida, A.; Graziani, C.; Fenimore, E. E.; Donaghy, T. Q.; Matsuoka, M.; Suzuki, M.; Ricker, G.; Atteia, J. L.; Shirasaki, Y.; Tamagawa, T.; Torii, K.; Galassi, M.; Doty, J.; Vanderspek, R.; Crew, G. B.; Villasenor, J.; Butler, Nathaniel; Prigozhin, G.; Jernigan, J. G.; Barraud, C.; Boer, M.; Dezalay, J. P.; Olive, J. F.; Hurley, K.; Levine, A.; Monnelly, G.; Martel, F.; Morgan, E.; Woosley, S. E.; Cline, T.; Braga, J.; Manchanda, R.; Pizzichini, G.; Takagishi, K.; Yamauchi, M.

In: Astrophysical Journal, Vol. 629, No. 1 I, 10.08.2005, p. 311-327.

Research output: Contribution to journalArticle

Sakamoto, T, Lamb, DQ, Kawai, N, Yoshida, A, Graziani, C, Fenimore, EE, Donaghy, TQ, Matsuoka, M, Suzuki, M, Ricker, G, Atteia, JL, Shirasaki, Y, Tamagawa, T, Torii, K, Galassi, M, Doty, J, Vanderspek, R, Crew, GB, Villasenor, J, Butler, N, Prigozhin, G, Jernigan, JG, Barraud, C, Boer, M, Dezalay, JP, Olive, JF, Hurley, K, Levine, A, Monnelly, G, Martel, F, Morgan, E, Woosley, SE, Cline, T, Braga, J, Manchanda, R, Pizzichini, G, Takagishi, K & Yamauchi, M 2005, 'Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2', Astrophysical Journal, vol. 629, no. 1 I, pp. 311-327. https://doi.org/10.1086/431235
Sakamoto T, Lamb DQ, Kawai N, Yoshida A, Graziani C, Fenimore EE et al. Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2. Astrophysical Journal. 2005 Aug 10;629(1 I):311-327. https://doi.org/10.1086/431235
Sakamoto, T. ; Lamb, D. Q. ; Kawai, N. ; Yoshida, A. ; Graziani, C. ; Fenimore, E. E. ; Donaghy, T. Q. ; Matsuoka, M. ; Suzuki, M. ; Ricker, G. ; Atteia, J. L. ; Shirasaki, Y. ; Tamagawa, T. ; Torii, K. ; Galassi, M. ; Doty, J. ; Vanderspek, R. ; Crew, G. B. ; Villasenor, J. ; Butler, Nathaniel ; Prigozhin, G. ; Jernigan, J. G. ; Barraud, C. ; Boer, M. ; Dezalay, J. P. ; Olive, J. F. ; Hurley, K. ; Levine, A. ; Monnelly, G. ; Martel, F. ; Morgan, E. ; Woosley, S. E. ; Cline, T. ; Braga, J. ; Manchanda, R. ; Pizzichini, G. ; Takagishi, K. ; Yamauchi, M. / Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2. In: Astrophysical Journal. 2005 ; Vol. 629, No. 1 I. pp. 311-327.
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abstract = "We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first 3 years of its mission, focusing on the properties of X-ray flashes (XRFs) and X-ray-rich GRBs (XRRs). We find that the numbers of XRFs, XRRs, and GRBs are comparable, and that the durations and the sky distributions of XRFs and XRRs are similar to those of GRBs. We also find that the spectral properties of XRFs and XRRs are similar to those of GRBs, except that the values of the peak energy Epeak obs of the burst spectrum in vFv, the peak energy flux Fpeak, and the energy fluence SE of XRFs are much smaller (and those of XRRs are smaller) than those of GRBs. Finally, we find that the distributions of all three kinds of bursts form a continuum in the [SE(2-30 keV), S E(30-400) keV] plane, the [SE(2-400 keV), E peak] plane, and the [Fpeak(50-300 keV), E peak] plane. These results provide strong evidence that all three kinds of bursts arise from the same phenomenon.",
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TY - JOUR

T1 - Global characteristics of X-ray flashes and X-ray-rich gamma-ray bursts observed by HETE-2

AU - Sakamoto, T.

AU - Lamb, D. Q.

AU - Kawai, N.

AU - Yoshida, A.

AU - Graziani, C.

AU - Fenimore, E. E.

AU - Donaghy, T. Q.

AU - Matsuoka, M.

AU - Suzuki, M.

AU - Ricker, G.

AU - Atteia, J. L.

AU - Shirasaki, Y.

AU - Tamagawa, T.

AU - Torii, K.

AU - Galassi, M.

AU - Doty, J.

AU - Vanderspek, R.

AU - Crew, G. B.

AU - Villasenor, J.

AU - Butler, Nathaniel

AU - Prigozhin, G.

AU - Jernigan, J. G.

AU - Barraud, C.

AU - Boer, M.

AU - Dezalay, J. P.

AU - Olive, J. F.

AU - Hurley, K.

AU - Levine, A.

AU - Monnelly, G.

AU - Martel, F.

AU - Morgan, E.

AU - Woosley, S. E.

AU - Cline, T.

AU - Braga, J.

AU - Manchanda, R.

AU - Pizzichini, G.

AU - Takagishi, K.

AU - Yamauchi, M.

PY - 2005/8/10

Y1 - 2005/8/10

N2 - We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first 3 years of its mission, focusing on the properties of X-ray flashes (XRFs) and X-ray-rich GRBs (XRRs). We find that the numbers of XRFs, XRRs, and GRBs are comparable, and that the durations and the sky distributions of XRFs and XRRs are similar to those of GRBs. We also find that the spectral properties of XRFs and XRRs are similar to those of GRBs, except that the values of the peak energy Epeak obs of the burst spectrum in vFv, the peak energy flux Fpeak, and the energy fluence SE of XRFs are much smaller (and those of XRRs are smaller) than those of GRBs. Finally, we find that the distributions of all three kinds of bursts form a continuum in the [SE(2-30 keV), S E(30-400) keV] plane, the [SE(2-400 keV), E peak] plane, and the [Fpeak(50-300 keV), E peak] plane. These results provide strong evidence that all three kinds of bursts arise from the same phenomenon.

AB - We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first 3 years of its mission, focusing on the properties of X-ray flashes (XRFs) and X-ray-rich GRBs (XRRs). We find that the numbers of XRFs, XRRs, and GRBs are comparable, and that the durations and the sky distributions of XRFs and XRRs are similar to those of GRBs. We also find that the spectral properties of XRFs and XRRs are similar to those of GRBs, except that the values of the peak energy Epeak obs of the burst spectrum in vFv, the peak energy flux Fpeak, and the energy fluence SE of XRFs are much smaller (and those of XRRs are smaller) than those of GRBs. Finally, we find that the distributions of all three kinds of bursts form a continuum in the [SE(2-30 keV), S E(30-400) keV] plane, the [SE(2-400 keV), E peak] plane, and the [Fpeak(50-300 keV), E peak] plane. These results provide strong evidence that all three kinds of bursts arise from the same phenomenon.

KW - Gamma rays: bursts

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