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AMIGO - The Astrodynamical Middle-frequency Interferometric GW(Gravitation-Wave) Observatory is a first-generation mid-frequency GW missionbridging the sensitivity gap between the high-frequency GW detectors andlow-frequency space GW detectors. In our previous works, we have obtainedappropriate heliocentric orbit formations of nominal arm length 10,000 km withtheir first-generation time-delay configurations satisfying frequency noisereduction requirement, and we have also worked out thrust-fuel friendlyconstant-arm heliocentric orbit formations. In this paper, we review and studynoise requirements and present the corresponding GW sensitivities. From thedesign white position noises and acceleration noises, we obtain the GWsensitivities for the first-generation Michelson X TDI configuration of b-AMIGO(baseline AMIGO), AMIGO, and e-AMIGO (enhanced AMIGO). In view of the currenttechnology development, we study and indicate steps to implement the AMIGOmission concept.

Core Noise Requirements, and GW Sensitivities of AMIGO