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GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

机译：GWTC-1：在第一和第二次观察运行期间，Ligo和Virgo观察到的紧凑型二元合并的重力波瞬态目录

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We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1 M ⊙ during the first and second observing runs of the advanced gravitational-wave detector network. During the first observing run ( O 1 ), from September 12, 2015 to January 19, 2016, gravitational waves from three binary black hole mergers were detected. The second observing run ( O 2 ), which ran from November 30, 2016 to August 25, 2017, saw the first detection of gravitational waves from a binary neutron star inspiral, in addition to the observation of gravitational waves from a total of seven binary black hole mergers, four of which we report here for the first time: GW170729, GW170809, GW170818, and GW170823. For all significant gravitational-wave events, we provide estimates of the source properties. The detected binary black holes have total masses between 18.6 ? 0.7 + 3.2 M ⊙ and 84.4 ? 11.1 + 15.8 M ⊙ and range in distance between 320 ? 110 + 120 and 2840 ? 1360 + 1400 Mpc . No neutron star–black hole mergers were detected. In addition to highly significant gravitational-wave events, we also provide a list of marginal event candidates with an estimated false-alarm rate less than 1?per 30?days. From these results over the first two observing runs, which include approximately one gravitational-wave detection per 15?days of data searched, we infer merger rates at the 90% confidence intervals of 110 ? 3840 Gpc ? 3 y ? 1 for binary neutron stars and 9.7 ? 101 Gpc ? 3 y ? 1 for binary black holes assuming fixed population distributions and determine a neutron star–black hole merger rate 90% upper limit of 610 Gpc ? 3 y ? 1 .
机译：我们在先进的引力波检测器网络的第一和第二观察运行期间，将三个重力波搜索的结果从三个和第二观察运行期间与高于1毫升的组件质量进行结合。在2016年9月12日至2016年1月19日至19日至1月19日的第一次观察运行期间，检测到三个二进制黑洞并购的引力波。 2016年11月30日至2017年8月25日从二元中子星的第一次检测到从总量的七个二进制的观察到重力的观察外，第二次观察运行（O 2）黑洞兼并，其中四个我们首次报告：GW170729，GW170809，GW170818和GW170823。对于所有重要的重力波事件，我们提供源属性的估计。检测到的二进制黑洞的总质量在18.6之间？ 0.7 + 3.2 m⊙和84.4？ 11.1 + 15.8 m⊙和320之间的距离范围？ 110 + 120和2840？ 1360 + 1400 MPC。没有检测到中子星形黑洞并发件。除了高度重要的引力波事件外，还提供了边际事件候选列表，估计的假警报率小于1？每30天。从这些结果，在前两个观察运行中，包括每15个数据的大约一个重力波检测，我们在110的90％置信区间推断合并率？ 3840 GPC？ 3 y？ 1为二元中子恒星和9.7？ 101 GPC？ 3 y？ 1对于二进制黑洞假设固定人口分布并确定中子星黑洞合并率为90％的上限610 gpc？ 3 y？ 1。

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    《Physical Review X》 |2019年第3期|共49页
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