JIGI achieves about four orders of magnitude sensitivity gain in the 0.1-0.3 Hz band by using repeated free-fall test masses to remove seismic and suspension noise, with analysis of detrending for actuation noise.
Kuroyanagi, et al., Probing the Universe through the stochastic gravitational wave background, Journal of Cosmology and Astroparticle Physics (2018) 038
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Jiggled interferometer: Ground-based gravitational wave detector using rapidly-repeated free-falling test masses
JIGI achieves about four orders of magnitude sensitivity gain in the 0.1-0.3 Hz band by using repeated free-fall test masses to remove seismic and suspension noise, with analysis of detrending for actuation noise.