CIGO and TCIGO lunar detectors achieve superior sky localization for 0.1-10 Hz gravitational waves compared to TianQin and LISA when noise mitigation succeeds, with TCIGO offering five-fold improvement.
Thez-axis is taken to be parallel to the lunar polar axis, while thex–yplane coincides with the lunar orbital plane
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The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
CIGO and TCIGO lunar detectors achieve superior sky localization for 0.1-10 Hz gravitational waves compared to TianQin and LISA when noise mitigation succeeds, with TCIGO offering five-fold improvement.