“…For the calibration of A = 10 6 amplifier is convenient to use shot 34 or thermal noise. 35 The rectified signal is collected on the lock-in capacitors for, say, ∆t = 5 s. Evaluating the electric voltage noise of the first operational amplifiers of the pre-amplifier to have spectral density parameter e N = 1.2, nV/ √ Hz, typical noise voltage can be evaluated as U N = e N √ ∆t = 2.68 nV we obtain Bernoulli signal to noise ratio r S/N = 3.39, which reveals that experiment is doable, and Cooper pair mass in cuprates can be determined using standard electronic equipment.…”