Atomic Interferometric Gravitational-Wave Space Observatory (AIGSO)

Gao Dong-Feng^{1, 2, †}, Wang Jin^{1, 2}, Zhan Ming-Sheng^{1, 2, ‡}

Strain density for several potential GW sources. A signal-to-noise ratio of 5 is assumed. For comparison, the sensitivity curves for AIGSO with T = 1 s and 10 s are also shown.