SWIFT GRB GRB071010B: OUTLIER OF THE E-peak(src)-E-gamma AND E-iso-E-peak(src)-t(jet)(src) CORRELATIONS

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/27871

Title:	SWIFT GRB GRB071010B: OUTLIER OF THE E-peak(src)-E-gamma AND E-iso-E-peak(src)-t(jet)(src) CORRELATIONS
Authors:	Urata,Y;Huang,KY;Im,M;Lee,I;Deng,JS;Ip,W;Krimm,H;Liping,X;Ohno,M;Qiu,YL;Sugita,S;Tashiro,M;Wei,JY;Yamaoka,K;Zheng,WK
Contributors:	天文研究所
Keywords:	GAMMA-RAY BURSTS;FOLLOW-UP OBSERVATIONS;SHALLOW DECAY;AFTERGLOWS;LUMINOSITY;EMISSION;SPECTRA;SYSTEM;ENERGY;BREAKS
Date:	2009
Issue Date:	2010-06-29 19:35:12 (UTC+8)
Publisher:	中央大學
Abstract:	We present multi-band results for GRB071010B based on Swift, Suzaku, and ground-based optical observations. This burst is an ideal target to evaluate the robustness of the E-peak(src) - E-iso and E-peak(src) - E-gamma relations, whose studies have been in stagnation due to the lack of the combined estimation of E-peak(src) and long-term optical monitoring. The joint prompt spectral fitting using Swift/Burst Alert Telescope and Suzaku/Wide-band All-sky Monitor data yielded the spectral peak energy as E-peak(src) of 86.5(-6.3)(+6.4) keV and E-iso of 2.25(-0.16)(+0.19) x 10(52) erg with z = 0.947. The optical afterglow light curve is well fitted by a simple power law with temporal index alpha = -0.60 +/- 0.02. The lower limit of temporal break in the optical light curve is 9.8 days. Our multi-wavelength analysis reveals that GRB071010B follows E-peak(src) - E-iso but violates the E-peak(src) - E-gamma and E-iso - E-peak(src) - t(jet)(src) at more than the 3 sigma level.
Relation:	ASTROPHYSICAL JOURNAL LETTERS
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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