2010
DOI: 10.1051/0004-6361/201014272
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Infrared/optical – X-ray simultaneous observations of X-ray flares in GRB 071112C and GRB 080506

Abstract: Aims. We investigate the origin of short X-ray flares which are occasionally observed in early stages of afterglows of gamma-ray bursts (GRBs). Methods. We observed two Swift events, GRB 071112C and GRB 080506, before the start of X-ray flares in the optical and nearinfrared (NIR) bands with the 1.5-m Kanata telescope. In conjunction with published X-ray and optical data, we analyzed densely sampled light curves of the early afterglows and spectral energy distributions (SEDs) in the NIR-X-ray ranges. Results. … Show more

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Cited by 11 publications
(7 citation statements)
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“…Fortunately, there is no significant color change between our R-and I-band measurements. An achromatic NIR evolution was also reported by Uehara et al (2010), and which supports our optical results and indicates achromatic evolution in the Rand I-band light curves. The peak in the R band is thus unlikely due to the passage of the synchrotron peak.…”
Section: Early Bump In Optical Light Curvesupporting
confidence: 92%
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“…Fortunately, there is no significant color change between our R-and I-band measurements. An achromatic NIR evolution was also reported by Uehara et al (2010), and which supports our optical results and indicates achromatic evolution in the Rand I-band light curves. The peak in the R band is thus unlikely due to the passage of the synchrotron peak.…”
Section: Early Bump In Optical Light Curvesupporting
confidence: 92%
“…If we exclude the flare component, the overall XRT light curve could be well fit by a single power law with an index α x = 1.36 ± 0.02. The afterglow decayed with an index of −1.36, consistent with the analysis of Uehara et al (2010). A flare occurred around t = 500 s following the burst and approached the original maximum brightness of 4.23 μJy.…”
Section: Optical and X-ray Temporal Analysissupporting
confidence: 82%
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“…Most rebrightenings are only observed in the X-ray band. Some early X-ray bumps, usually called X-ray flares, have no corresponding optical features (see the statistics by Melandri et al 2008 andRykoff et al 2009, as well as Uehara et al 2010, for the individual cases of GRB 071112C and GRB 080506). In contrast, but less frequently, a rebrightening feature may be seen in the optical but not in the X-ray band (e.g.…”
Section: Introductionmentioning
confidence: 99%