Challenges in space-based gravitational wave data analysis and applications of artificial intelligence
(Color online) The design sensitivity curves and primary target sources of the space-based gravitational wave detectors LISA, Taiji, and TianQin. The sensitivity of each detector is the total sensitivity of the first-generation Michelson-AET channel under the equal-arm-length approximation, expressed in terms of characteristic strain. The dashed curves represent the sensitivities resulting from instrumental noise (according to the noise requirements of LISA [11], Taiji [18], and TianQin [21]), while the solid curves represent the results after incorporating the galactic foreground noise.
