IGEC2: A 17-month search for gravitational wave bursts in 2005-2007
IGEC2: A 17-month search for gravitational wave bursts in 2005-2007
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IGEC2：2005-2007 年为期 17 个月的引力波爆发搜索
DOI：
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发表时间：
2010
期刊：
影响因子：
--
通讯作者：
P. Zhang
中科院分区：
文献类型：
--
作者：
P. Astone;L. Baggio;M. Bassan;M. Bignotto;M. Bonaldi;P. Bonifazi;G. Cavallari;M. Cerdonio;E. Coccia;L. Conti;S. D’Antonio;M. Emilio;M. Drago;V. Fafone;P. Falferi;S. Foffa;P. Fortini;S. Frasca;G. Giordano;W. Hamilton;J. Hanson;W. Johnson;N. Liguori;S. Longo;M. Maggiore;F. Marin;A. Marini;M. McHugh;R. Mezzena;P. Miller;Y. Minenkov;A. Mion;G. Modestino;A. Moleti;D. Nettles;A. Ortolan;G. Pallottino;G. Pizzella;S. Poggi;G. Prodi;V. Re;A. Rocchi;F. Ronga;F. Salemi;R. Sturani;L. Taffarello;R. Terenzi;G. Vedovato;A. Vinante;M. Visco;S. Vitale;J. Weaver;J. Zendri;P. Zhang
本文介绍IGEC 2天文台对引力波短爆发进行515天搜索的结果。该网络包括4个低温共振棒探测器：欧洲的AURIGA、EXPLORER和NAUTILUS，以及美国的ALLEGRO。这些结果涵盖了从2005年11月6日到2007年4月15日的时间段，部分重叠了LIGO干涉仪探测器的第一次长期观测。天文台以高占空比运行，即四次重合观测占空比为57%，三次重合观测占空比为94%。灵敏度是有史以来最好的酒吧网络：我们可以检测到，效率> 50%，脉冲事件与突发应变振幅h{sub rss} <或约。1x10{sup -19} Hz{sup -1/2}。网络数据分析基于至少三个检测器上的时间重合搜索，使用盲搜索技术，并被调整以实现1/世纪的误报率。当遮蔽被移除时，没有发现引力波候选者。
We present here the results of a 515 day search for short bursts of gravitational waves by the IGEC2 observatory. This network included 4 cryogenic resonant-bar detectors: AURIGA, EXPLORER, and NAUTILUS in Europe, and ALLEGRO in America. These results cover the time period from November 6th 2005 until April 15th 2007, partly overlapping the first long term observations by the LIGO interferometric detectors. The observatory operated with high duty cycle, namely, 57% for fourfold coincident observations, and 94% for threefold observations. The sensitivity was the best ever obtained by a bar network: we could detect, with an efficiency >50%, impulsive events with a burst strain amplitude h{sub rss} < or approx. 1x10{sup -19} Hz{sup -1/2}. The network data analysis was based on time coincidence searches over at least three detectors, used a blind search technique, and was tuned to achieve a false alarm rate of 1/century. When the blinding was removed, no gravitational wave candidate was found.
在第四次科学运行的 LIGO 数据中搜索引力波爆发
影响因子：
3.5
作者：
Abbott B
通讯作者：
Abbott B