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SWIFT IDENTIFICATION OF DARK GAMMA-RAY BURSTS

机译:黑暗伽马射线爆发的SWIFT识别

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摘要

We present an optical flux versus X-ray flux diagram for all known gamma-ray bursts (GRBs) for which an X-ray afterglow has been detected. We propose an operational definition of dark bursts as (hose bursts that arc optically subluminous with respect to the fireball model, i.e., that have an optical-to-X-ray spectral index β_(ox) < 0.5. Out of a sample of 52 GRBs, we identify five dark bursts. The definition and diagram serve as a simple and quick diagnostic tool for identifying dark GRBs based on limited information, particularly useful for early and objective identification of dark GRBs observed with the Swift satellite.
机译:我们提供了所有已知的X射线余辉已被检测到的伽马射线暴(GRB)的光通量与X射线通量的关系图。我们提出暗脉冲的操作定义为(相对于火球模型在光学上为亚光的软管脉冲,即,其光学对X射线光谱指数β_(ox)<0.5。在52个样本中GRB,我们识别出五个暗脉冲,该定义和图表是基于有限信息识别暗GRB的简单快速的诊断工具,特别适用于早期和客观识别Swift卫星观测到的暗GRB。

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