The LISA-Taiji network

Abstract

Both LISA and Taiji, planned space-based gravitational-wave detectors in orbit around the Sun, are expected to launch in 2030-2035. Assuming a one-year overlap, we explore a potential LISA-Taiji network to fast and accurately localize the gravitational-wave sources.

6 pages. 2 figures

References in corpus (3)

• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Laser Interferometer Space Antenna
• Localizing coalescing massive black hole binaries with gravitational waves

Cited by in corpus (13)

• Concepts and status of Chinese space gravitational wave detection projects
• The Gravitational-Wave Physics II: Progress
• Measuring Parity Violation in the Stochastic Gravitational Wave Background with the LISA-Taiji network
• Ultra-compact X-ray binaries with He star companions
• Observing gravitational wave polarizations with LISA-TAIJI network
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• Detection of gravitational waves in circular particle accelerators
• Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
• Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
• Geometric tilt-to-length coupling in precision interferometry: mechanisms and analytical descriptions
• Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background