most citedA waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism

179 citations · 219 across the 5 of their papers we have counts for

collaborators

9 papers

gr-qc20201 cited

Investigating eccentricities of the binary black hole signals from the LIGO-Virgo catalog GWTC-1

Qian-Yun Yun, Wen-Biao Han, Gang Wang +1

In the first Gravitational-Wave Transient Catalogue of LIGO and Virgo, all events are announced having zero eccentricity. In the present paper, we investigate the performance of SE…

gr-qc2020

Numerical simulation of sky localization for LISA-TAIJI joint observation

Gang Wang, Wei-Tou Ni, Wen-Biao Han +2

LISA is considered to be launched alongside the Athena to probe the energetic astrophysical processes. LISA can determine the direction of sources for Athena's follow-up observatio…

gr-qc2018

Gravitational wave emission under general parametrized metric from extreme mass ratio inspirals

Shuo Xin, Wen-Biao Han, Shu-Cheng Yang

Future space-borne interferometers will be able to detect gravitational waves at to Hz. At this band extreme-mass-ratio inspirals (EMRIs) can be promising gravi…

gr-qc2018

Testing dispersion of gravitational waves from eccentric extreme-mass-ratio inspirals

Shu-Cheng Yang, Wen-Biao Han, Shuo Xin +1

In general relativity, there is no dispersion in gravitational waves, while some modified gravity theories predict dispersion phenomena in the propagation of gravitational waves. I…

astro-ph.IM201716 cited

Advanced relativistic VLBI model for geodesy

Michael Soffel, Sergei Kopeikin, Wen-Biao Han

Our present relativistic part of the geodetic VLBI model for Earthbound antennas is a consensus model which is considered as a standard for processing high-precision VLBI observati…

gr-qc201714 cited

Excitation of high frequency voices from intermediate-mass-ratio inspirals with large eccentricity

Wen-Biao Han, Zhoujian Cao, Yi-Ming Hu

The coalescence of a stellar-mass compact object together with an intermediate-mass black hole, also known as intermediate-mass-ratio inspiral, is usually not expected to be a viab…