Likelihood for a network of gravitational-wave detectors with correlated noise

被引：0

作者：

Cireddu, Francesco ^{[1
,2
,3
]}

Wils, Milan ^{[1
,2
]}

Wong, Isaac C. F. ^{[1
,4
,5
]}

Pang, Peter T. H. ^{[6
,7
]}

Li, Tjonnie G. F. ^{[1
,2
,5
]}

Del Pozzo, Walter ^{[3
,8
]}

机构：

[1] Katholieke Univ Leuven, Leuven Grav Inst, Dept Mech Engn, Celestijnenlaan 200D Box 2415, B-3001 Leuven, Belgium

[2] Katholieke Univ Leuven, Dept Phys & Astron, Lab Semicond Phys, B-3001 Leuven, Belgium

[3] Univ Pisa, Dipartimento Fis E Fermi, I-56127 Pisa, Italy

[4] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, New Territories, Peoples R China

[5] Katholieke Univ Leuven, STADIUS Ctr Dynam Syst Signal Proc & Data Analyt, Dept Elect Engn ESAT, B-3001 Leuven, Belgium

[6] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands

[7] Univ Utrecht, Inst Gravitat & Subatom Phys GRASP, Princetonpl 1, NL-3584 CC Utrecht, Netherlands

[8] INFN, Sez Pisa, I-56127 Pisa, Italy

来源：

PHYSICAL REVIEW D | 2024年 / 110卷 / 10期

基金：

比利时弗兰德研究基金会;

关键词：

PARAMETER-ESTIMATION;

D O I：

10.1103/PhysRevD.110.104060

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Einstein Telescope faces a critical data analysis challenge with correlated noise, often overlooked in current parameter estimation analyses. We address this issue by presenting the statistical formulation of the likelihood that includes correlated noise for the Einstein Telescope or any detector network. By considering varying degrees of correlation, we probe the impact of noise correlations on the parameter estimation analysis of a GW150914-like event. We show that neglecting these correlations may significantly reduce the accuracy of the chirp mass reconstruction. This emphasizes how critical a proper treatment of correlated noise is, as presented in this work, to unlocking the wealth of results promised by the Einstein Telescope.

引用

页数：11