The Amaldi 10 Parallel Session C2 on gravitational wave (GW) search results, data analysis and parameter estimation included three lively sessions of lectures by 13 presenters, and 34 posters. The talks and posters covered a huge range of material, including results and analysis techniques for ground-based GW detectors, targeting anticipated signals from different astrophysical sources: compact binary inspiral, merger and ringdown; GW bursts from intermediate mass binary black hole mergers, cosmic string cusps, core-collapse supernovae, and other unmodeled sources; continuous waves from spinning neutron stars; and a stochastic GW background. There was considerable emphasis on Bayesian techniques for estimating the parameters of coalescing compact binary systems from the gravitational waveforms extracted from the data from the advanced detector network. This included methods to distinguish deviations of the signals from what is expected in the context of General Relativity.

中文翻译：

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引力波：搜索结果、数据分析和参数估计


关于引力波（GW）搜索结果、数据分析和参数估计的Amaldi 10平行会议C2包括由13名演讲者和34名海报组成的三场生动的讲座。演讲和海报涵盖了大量材料，包括地面引力波探测器的结果和分析技术，针对来自不同天体物理来源的预期信号：紧凑的双星螺旋、合并和振铃； GW从中等质量双黑洞合并、宇宙弦尖点、核心塌缩超新星和其他未建模的来源爆发；旋转中子星产生的连续波；和随机 GW 背景。人们相当重视贝叶斯技术，用于根据从先进探测器网络的数据中提取的重力波形来估计合并紧凑双星系统的参数。这包括区分信号与广义相对论背景下预期偏差的方法。