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 (6)

• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Laser Interferometer Space Antenna
• Angular Resolution of the LISA Gravitational Wave Detector
• The Afterglow of Massive Black Hole Coalescence
• Charge-induced force-noise on free-falling test masses: results from LISA Pathfinder
• Localizing coalescing massive black hole binaries with gravitational waves

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