“…For long-duration GW signals, these imprints accumulate over time, eventually giving rise to observable deviations which can be used to infer the GW amplitude, turning the binary into a dynamical GW detector. This idea has a long history [19][20][21][22][23][24][25][26][27][28][29][30][31][32][33], and has been used to search for GWs with the orbit of the binary pulsar B1913+16 [34]. 1 Nonetheless, this binary GW resonance effect has received relatively little attention in the GW community, and, we feel, has not yet been exploited to its full potential.…”