The 2005 october multiwavelength campaign of GRS 1915+105

Y. Ueda; R. Ishioka; K. Sekiguchi; M. Ribo; J. Rodriguez; S. Chaty; J. Greiner; G. Sala; Y. Fuchs; P. Goldoni; S. Covino; G. G. Pooley; P. Edwards; A. Tzioumis; H. Lehto; E. Gerard; P. Colom; J. Martin; S. A. Trushkin; A. J. Castro-Tirado; D. Hannikainen; H. Sudo; M. Honma; F. Iwamuro; K. Kubuta; K. Yamaoka; C. Done; S. Naik; Y. Fukazawa; L. Angelini; H. Awaki; K. Ebisawa; K. Iwasawa; N. Kawai; K. Kinugasa; M. Kokubun; T. Kotani; A. Kubota; T. Murakami; M. Namiki; H. Takahashi; T. Yaqoob; D. Yonetoku; A. Yoshida

The 2005 october multiwavelength campaign of GRS 1915+105

Y. Ueda
, R. Ishioka
, K. Sekiguchi
, M. Ribo
, J. Rodriguez
, S. Chaty
, J. Greiner
, G. Sala
, Y. Fuchs
, P. Goldoni
, S. Covino
, G. G. Pooley
, P. Edwards
, A. Tzioumis
, H. Lehto
, E. Gerard
, P. Colom
, J. Martin
, S. A. Trushkin
, A. J. Castro-Tirado

D. Hannikainen, H. Sudo, M. Honma, F. Iwamuro, K. Kubuta, K. Yamaoka, C. Done, S. Naik, Y. Fukazawa, L. Angelini, H. Awaki, K. Ebisawa, K. Iwasawa, N. Kawai, K. Kinugasa, M. Kokubun, T. Kotani, A. Kubota, T. Murakami, M. Namiki, H. Takahashi, T. Yaqoob, D. Yonetoku, A. Yoshida

Kyoto University
NAOJ
University of Barcelona
Institut Pierre Simon Laplace, CNRS and CEA
Laboratoire de Probabilités et Modèles Aléatoires
Max Planck Institut für Extraterrestrische Physik
Astroparticule and Cosmol APC
Istituto di Astrofisica e Planetologia Spaziali (IAPS)
University of Cambridge
Commonwealth Scientific and Industrial Research Organization
University of Turku
Sorbonne Univ.
SAO
Instituto de Astrofísica de Andalucía-CSIC
University of Helsinki
Gifu University
National Astronomical Observatory
Aoyama Gakuin University
Durham University
ISAS/JAXA
Hiroshima University
GSFC Laboratory for Atmopsheres
Ehime University
Tokyo Institute of Technology
Gunma Astronomical Observatory
University of Tokyo
Riken
Kanazawa University
Osaka University
Johns Hopkins University

Résultats de recherche: Contribution à un journal › Article de conférence › Revue par des pairs

Résumé

We report the first results of a large multiwavelength campaign of GRS 1915+105 performed between 2005 October 16 to October 18 with Suzaku, INTEGRAL, RXTE, Swift, Spitzer, and ground observatories including Subaru, ESO/NTT, REM (infrared), VLA, ATCA, Nancay, Ryle, and RATAN (radio). GRS 1915+105 was firstly in the stable state with a 6 Hz QPO but then entered into the oscillation phase identified as Class θ. The Suzaku spectra in the 1-80 keV band are very soft, approximated by a photo index of 3-3.8 with varying iron-K features in different Xray states. The simultaneous Subaru and X-ray light curves in the oscillation phase indicate that infrared flares occur after the X-ray dip with variable time delay. This result strongly suggests that the disc transition from State C to State A triggers the ejection of jet, which eventually produces infrared/radio flares by internal shock.

langue originale	Anglais
journal	International Conference Recent Advances in Natural Language Processing, RANLP
état	Publié - 1 janv. 2006
Modification externe	Oui
Evénement	6th Microquasar Workshop: Microquasars and Beyond, MQW 2006 - Como, Italie Durée: 18 sept. 2006 → 22 sept. 2006

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Ueda, Y., Ishioka, R., Sekiguchi, K., Ribo, M., Rodriguez, J., Chaty, S., Greiner, J., Sala, G., Fuchs, Y., Goldoni, P., Covino, S., Pooley, G. G., Edwards, P., Tzioumis, A., Lehto, H., Gerard, E., Colom, P., Martin, J., Trushkin, S. A., ... Yoshida, A. (2006). The 2005 october multiwavelength campaign of GRS 1915+105. International Conference Recent Advances in Natural Language Processing, RANLP.

@article{fa1a07ed738e4676aceef99ac0662198,

title = "The 2005 october multiwavelength campaign of GRS 1915+105",

abstract = "We report the first results of a large multiwavelength campaign of GRS 1915+105 performed between 2005 October 16 to October 18 with Suzaku, INTEGRAL, RXTE, Swift, Spitzer, and ground observatories including Subaru, ESO/NTT, REM (infrared), VLA, ATCA, Nancay, Ryle, and RATAN (radio). GRS 1915+105 was firstly in the stable state with a 6 Hz QPO but then entered into the oscillation phase identified as Class θ. The Suzaku spectra in the 1-80 keV band are very soft, approximated by a photo index of 3-3.8 with varying iron-K features in different Xray states. The simultaneous Subaru and X-ray light curves in the oscillation phase indicate that infrared flares occur after the X-ray dip with variable time delay. This result strongly suggests that the disc transition from State C to State A triggers the ejection of jet, which eventually produces infrared/radio flares by internal shock.",

author = "Y. Ueda and R. Ishioka and K. Sekiguchi and M. Ribo and J. Rodriguez and S. Chaty and J. Greiner and G. Sala and Y. Fuchs and P. Goldoni and S. Covino and Pooley, \{G. G.\} and P. Edwards and A. Tzioumis and H. Lehto and E. Gerard and P. Colom and J. Martin and Trushkin, \{S. A.\} and Castro-Tirado, \{A. J.\} and D. Hannikainen and H. Sudo and M. Honma and F. Iwamuro and K. Kubuta and K. Yamaoka and C. Done and S. Naik and Y. Fukazawa and L. Angelini and H. Awaki and K. Ebisawa and K. Iwasawa and N. Kawai and K. Kinugasa and M. Kokubun and T. Kotani and A. Kubota and T. Murakami and M. Namiki and H. Takahashi and T. Yaqoob and D. Yonetoku and A. Yoshida",

year = "2006",

month = jan,

day = "1",

language = "English",

journal = "International Conference Recent Advances in Natural Language Processing, RANLP",

issn = "1313-8502",

note = "6th Microquasar Workshop: Microquasars and Beyond, MQW 2006 ; Conference date: 18-09-2006 Through 22-09-2006",

}

Ueda, Y, Ishioka, R, Sekiguchi, K, Ribo, M, Rodriguez, J, Chaty, S, Greiner, J, Sala, G, Fuchs, Y, Goldoni, P, Covino, S, Pooley, GG, Edwards, P, Tzioumis, A, Lehto, H, Gerard, E, Colom, P, Martin, J, Trushkin, SA, Castro-Tirado, AJ, Hannikainen, D, Sudo, H, Honma, M, Iwamuro, F, Kubuta, K, Yamaoka, K, Done, C, Naik, S, Fukazawa, Y, Angelini, L, Awaki, H, Ebisawa, K, Iwasawa, K, Kawai, N, Kinugasa, K, Kokubun, M, Kotani, T, Kubota, A, Murakami, T, Namiki, M, Takahashi, H, Yaqoob, T, Yonetoku, D & Yoshida, A 2006, 'The 2005 october multiwavelength campaign of GRS 1915+105', International Conference Recent Advances in Natural Language Processing, RANLP.

TY - JOUR

T1 - The 2005 october multiwavelength campaign of GRS 1915+105

AU - Ueda, Y.

AU - Ishioka, R.

AU - Sekiguchi, K.

AU - Ribo, M.

AU - Rodriguez, J.

AU - Chaty, S.

AU - Greiner, J.

AU - Sala, G.

AU - Fuchs, Y.

AU - Goldoni, P.

AU - Covino, S.

AU - Pooley, G. G.

AU - Edwards, P.

AU - Tzioumis, A.

AU - Lehto, H.

AU - Gerard, E.

AU - Colom, P.

AU - Martin, J.

AU - Trushkin, S. A.

AU - Castro-Tirado, A. J.

AU - Hannikainen, D.

AU - Sudo, H.

AU - Honma, M.

AU - Iwamuro, F.

AU - Kubuta, K.

AU - Yamaoka, K.

AU - Done, C.

AU - Naik, S.

AU - Fukazawa, Y.

AU - Angelini, L.

AU - Awaki, H.

AU - Ebisawa, K.

AU - Iwasawa, K.

AU - Kawai, N.

AU - Kinugasa, K.

AU - Kokubun, M.

AU - Kotani, T.

AU - Kubota, A.

AU - Murakami, T.

AU - Namiki, M.

AU - Takahashi, H.

AU - Yaqoob, T.

AU - Yonetoku, D.

AU - Yoshida, A.

PY - 2006/1/1

Y1 - 2006/1/1

N2 - We report the first results of a large multiwavelength campaign of GRS 1915+105 performed between 2005 October 16 to October 18 with Suzaku, INTEGRAL, RXTE, Swift, Spitzer, and ground observatories including Subaru, ESO/NTT, REM (infrared), VLA, ATCA, Nancay, Ryle, and RATAN (radio). GRS 1915+105 was firstly in the stable state with a 6 Hz QPO but then entered into the oscillation phase identified as Class θ. The Suzaku spectra in the 1-80 keV band are very soft, approximated by a photo index of 3-3.8 with varying iron-K features in different Xray states. The simultaneous Subaru and X-ray light curves in the oscillation phase indicate that infrared flares occur after the X-ray dip with variable time delay. This result strongly suggests that the disc transition from State C to State A triggers the ejection of jet, which eventually produces infrared/radio flares by internal shock.

AB - We report the first results of a large multiwavelength campaign of GRS 1915+105 performed between 2005 October 16 to October 18 with Suzaku, INTEGRAL, RXTE, Swift, Spitzer, and ground observatories including Subaru, ESO/NTT, REM (infrared), VLA, ATCA, Nancay, Ryle, and RATAN (radio). GRS 1915+105 was firstly in the stable state with a 6 Hz QPO but then entered into the oscillation phase identified as Class θ. The Suzaku spectra in the 1-80 keV band are very soft, approximated by a photo index of 3-3.8 with varying iron-K features in different Xray states. The simultaneous Subaru and X-ray light curves in the oscillation phase indicate that infrared flares occur after the X-ray dip with variable time delay. This result strongly suggests that the disc transition from State C to State A triggers the ejection of jet, which eventually produces infrared/radio flares by internal shock.

UR - https://www.scopus.com/pages/publications/85133355229

M3 - Conference article

AN - SCOPUS:85133355229

SN - 1313-8502

JO - International Conference Recent Advances in Natural Language Processing, RANLP

JF - International Conference Recent Advances in Natural Language Processing, RANLP

T2 - 6th Microquasar Workshop: Microquasars and Beyond, MQW 2006

Y2 - 18 September 2006 through 22 September 2006

ER -

The 2005 october multiwavelength campaign of GRS 1915+105

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