Spectrum feature of the underlying soft component of GRB041006.

Y. Shirasaki, A. Yoshida, N. Kawai, Y. Nakagawa, T. Tamagawa, M. Suzuki, S. Sugita, I. Takahashi, M. Arimoto, T. Shimokawabe, N. Vasquez, T. Ishimura, R. Sato, T. Sakamoto, M. Kuwahara, M. Matsuoka

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.

Original languageEnglish
Title of host publicationGamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference
Pages158-161
Number of pages4
Volume1000
DOIs
Publication statusPublished - 2008
Externally publishedYes
EventSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM
Duration: 2007 Nov 52007 Nov 9

Other

OtherSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007
CitySanta Fe, NM
Period07/11/507/11/9

Fingerprint

energy bands
light curve
x rays

Keywords

  • GRB
  • GRB 041006
  • HETE2

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Shirasaki, Y., Yoshida, A., Kawai, N., Nakagawa, Y., Tamagawa, T., Suzuki, M., ... Matsuoka, M. (2008). Spectrum feature of the underlying soft component of GRB041006. In Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference (Vol. 1000, pp. 158-161) https://doi.org/10.1063/1.2943433

Spectrum feature of the underlying soft component of GRB041006. / Shirasaki, Y.; Yoshida, A.; Kawai, N.; Nakagawa, Y.; Tamagawa, T.; Suzuki, M.; Sugita, S.; Takahashi, I.; Arimoto, M.; Shimokawabe, T.; Vasquez, N.; Ishimura, T.; Sato, R.; Sakamoto, T.; Kuwahara, M.; Matsuoka, M.

Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. Vol. 1000 2008. p. 158-161.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Shirasaki, Y, Yoshida, A, Kawai, N, Nakagawa, Y, Tamagawa, T, Suzuki, M, Sugita, S, Takahashi, I, Arimoto, M, Shimokawabe, T, Vasquez, N, Ishimura, T, Sato, R, Sakamoto, T, Kuwahara, M & Matsuoka, M 2008, Spectrum feature of the underlying soft component of GRB041006. in Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. vol. 1000, pp. 158-161, Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007, Santa Fe, NM, 07/11/5. https://doi.org/10.1063/1.2943433
Shirasaki Y, Yoshida A, Kawai N, Nakagawa Y, Tamagawa T, Suzuki M et al. Spectrum feature of the underlying soft component of GRB041006. In Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. Vol. 1000. 2008. p. 158-161 https://doi.org/10.1063/1.2943433
Shirasaki, Y. ; Yoshida, A. ; Kawai, N. ; Nakagawa, Y. ; Tamagawa, T. ; Suzuki, M. ; Sugita, S. ; Takahashi, I. ; Arimoto, M. ; Shimokawabe, T. ; Vasquez, N. ; Ishimura, T. ; Sato, R. ; Sakamoto, T. ; Kuwahara, M. ; Matsuoka, M. / Spectrum feature of the underlying soft component of GRB041006. Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. Vol. 1000 2008. pp. 158-161
@inproceedings{d042f3baa04f484082cff98765eda28e,
title = "Spectrum feature of the underlying soft component of GRB041006.",
abstract = "GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.",
keywords = "GRB, GRB 041006, HETE2",
author = "Y. Shirasaki and A. Yoshida and N. Kawai and Y. Nakagawa and T. Tamagawa and M. Suzuki and S. Sugita and I. Takahashi and M. Arimoto and T. Shimokawabe and N. Vasquez and T. Ishimura and R. Sato and T. Sakamoto and M. Kuwahara and M. Matsuoka",
year = "2008",
doi = "10.1063/1.2943433",
language = "English",
isbn = "9780735405332",
volume = "1000",
pages = "158--161",
booktitle = "Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference",

}

TY - GEN

T1 - Spectrum feature of the underlying soft component of GRB041006.

AU - Shirasaki, Y.

AU - Yoshida, A.

AU - Kawai, N.

AU - Nakagawa, Y.

AU - Tamagawa, T.

AU - Suzuki, M.

AU - Sugita, S.

AU - Takahashi, I.

AU - Arimoto, M.

AU - Shimokawabe, T.

AU - Vasquez, N.

AU - Ishimura, T.

AU - Sato, R.

AU - Sakamoto, T.

AU - Kuwahara, M.

AU - Matsuoka, M.

PY - 2008

Y1 - 2008

N2 - GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.

AB - GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.

KW - GRB

KW - GRB 041006

KW - HETE2

UR - http://www.scopus.com/inward/record.url?scp=84874868869&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84874868869&partnerID=8YFLogxK

U2 - 10.1063/1.2943433

DO - 10.1063/1.2943433

M3 - Conference contribution

SN - 9780735405332

VL - 1000

SP - 158

EP - 161

BT - Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference

ER -