“…0 , with T sys being the system temperature, A the cross-sectional area, Q the quality factor, t the integration time-typically t ≲ 1 ms per subspectrum to mitigate 1/f noise, which are stacked into a single spectrum at each frequency to mitigate white noise [74]-and B 0 the magnetic field strength. Therefore, in addition to procuring a powerful superconducting solenoid with a large bore that allows for housing a lowtemperature cryostat with a large cross-sectional area-e.g., [68]-it becomes crucial to provide a high Q factor. The quality factor of a Fabry-Pérot resonator, defined as 2π times the ratio of the energy stored in the resonator and the energy loss per oscillation period, is Q = ωτ g , where the group delay time, τ g , is the average lifetime of a photon in the resonator or, equivalently, decay time of the energy density of radiation in the interferometer, and adopts typical values of a few nanoseconds per layer [75].…”