论文标题
多功能仪器爆发档案(Minbar)
The Multi-INstrument Burst ARchive (MINBAR)
论文作者
论文摘要
我们介绍了尚未组装的最大的I型(热核)X射线爆发样品,其中包括来自85个爆发源的7083次爆发。该样品是从1996年2月8日至2012年5月3日之间的长期卫星Rxte,Bepposax和Integrot的观测值中得出的,Bepposax和Integrove的观测值是从早期的目录和文献中组装的115个爆发源的全面目录中得出的。我们对每个爆发灯曲线(标准化为相对仪器有效区域)进行了一致的分析,并提供了上升时间,峰值强度,爆发时间尺度和频率的测量。对于使用RXTE/PCA和BEPPOSAX/WFC观察到的爆发,我们还提供了时间分辨光谱,包括降压峰值通量和通量的估计值,以及爆发峰处的光谱参数。对于从具有先前检测到的爆发振荡的源的PCA观察到的950次爆发,我们包括对高空分辨率数据的分析,提供有关振荡的可检测性和振幅的信息,以及在爆发中发现的位置。我们还介绍了对样品时间范围内爆发源的118848观察结果的分析。我们从大多数观察结果中提取了3-25 keV X射线光谱,并且(对于满足我们的信噪标准的观测值),我们提供了通量,光谱颜色的测量值,并且为选定的来源,对于最佳拟合光谱模型而言,颜色颜色图上的位置。我们介绍了样本的描述,迄今已完成的科学调查的摘要以及进一步研究的建议。
We present the largest sample of type-I (thermonuclear) X-ray bursts yet assembled, comprising 7083 bursts from 85 bursting sources. The sample is drawn from observations with Xenon-filled proportional counters on the long-duration satellites RXTE, BeppoSAX and INTEGRAL, between 1996 February 8, and 2012 May 3. The burst sources were drawn from a comprehensive catalog of 115 burst sources, assembled from earlier catalogs and the literature. We carried out a consistent analysis for each burst lightcurve (normalised to the relative instrumental effective area), and provide measurements of rise time, peak intensity, burst timescale, and fluence. For bursts observed with the RXTE/PCA and BeppoSAX/WFC we also provide time-resolved spectroscopy, including estimates of bolometric peak flux and fluence, and spectral parameters at the peak of the burst. For 950 bursts observed with the PCA from sources with previously detected burst oscillations, we include an analysis of the high-time resolution data, providing information on the detectability and amplitude of the oscillations, as well as where in the burst they are found. We also present analysis of 118848 observations of the burst sources within the sample timeframe. We extracted 3-25 keV X-ray spectra from most observations, and (for observations meeting our signal-to-noise criterion), we provide measurements of the flux, spectral colours, and for selected sources, the position on the colour-colour diagram, for the best-fit spectral model. We present a description of the sample, a summary of the science investigations completed to date, and suggestions for further studies.