Observing Supermassive Black Hole Binary Systems with LISA

被引：0
|
作者：
Trias, Miquel [1 ]
Sintes, Alicia M. [1 ]
机构：
[1] Univ Illes Balears, Dept Fis, E-07122 Palma de Mallorca, Spain
来源：
HIGHLIGHTS OF SPANISH ASTROPHYSICS V | 2010年
关键词：
D O I：
10.1007/978-3-642-11250-8_79
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study parameter estimation of supermassive black holes by LISA using the inspiral full post-Newtonian gravitational waveforms up to 2PN. The analysis shows that LISA will observe the coalescence of a system with total mass (10(4) - 10(8)) M-circle dot with signal-to-noise ratios of hundreds and errors in masses and luminosity distance smaller than 10%. For sources at z = 1 we find that at least 20% could be localized within a (1 degrees x 1 degrees) patch.
引用
收藏
页码：359 / 359
页数：1
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