The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
This paper demonstrates that the proposed lunar-based Crater Interferometry Gravitational-wave Observatory (CIGO) and its upgraded tetrahedral configuration (TCIGO) can significantly outperform existing space-based missions like TianQin and LISA in sky map resolution for monochromatic sources in the 0.1–10 Hz band, provided lunar noise is effectively mitigated.