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After first reviewing the gravitational wave (GW) spectral classification. wediscuss the sensitivities of GW detection in space aimed at low frequency band(100 nHz-100 mHz) and middle frequency band (100 mHz-10 Hz). The science goalsare to detect GWs from (i) Supermassive Black Holes; (ii) Extreme-Mass-RatioBlack Hole Inspirals; (iii) Intermediate-Mass Black Holes; (iv) GalacticCompact Binaries; (v) Stellar-Size Black Hole Binaries; and (vi) Relic GWBackground. The detector proposals have arm length ranging from 100 km to1.35x109 km (9 AU) including (a) Solar orbiting detectors and (b) Earthorbiting detectors. We discuss especially the sensitivities in the frequencyband 0.1-10 microHz and the middle frequency band (0.1 Hz-10 Hz). We proposeand discuss AMIGO as an Astrodynamical Middle-frequency Interferometric GWObservatory.

Gravitational Wave (GW) Classification, Space GW Detection Sensitivities and AMIGO (Astrodynamical Middle-frequency Interferometric GW Observatory)