To isolate the ON-bipolar cell component of the ERG (PII), the modeled PIII was subtracted from the raw waveform.
32 PII amplitudes measured at a fixed time of 70 ms were plotted as a function of luminous energy and modeled using a saturating hyperbolic function, as given in
Equation 2. The amplitude (
V, μV) as a function of luminous energy (
i, log cd.s.m
−2) is given by a maximal amplitude (
Vmax , μV), semisaturation constant (
k, log cd.s.m
−2), where sensitivity is 1/
k (cd
−1.s
−1.m
2) and
n is a dimensionless exponent that determines the slope of the function.
The dark-adapted ERG reflects contributions from both rod and cone pathways. Therefore,
Equation 2 was fit to luminous energies below those containing cone responses. This was determined by establishing the amplitude of the “putative” rod response from a twin-flash paradigm at 2.07 log cd.s.m
−2. By using a 500-ms interstimulus interval, the long refractory period of the rod system means that only cone responses are recorded in the second flash, which is then subtracted from the mixed response to return the putative rod response. Group data for rod amplitude (at 2.07 log cd.s.m
−2) was compared with the amplitude of mixed responses for all other luminous energies. Amplitudes for luminous energies greater than −0.82 log cd.s.m
−2 were found to be significantly larger than the isolated rod PII amplitude (
P < 0.05), indicating significant cone contribution. Thus,
Equation 2 was fit to luminous energies between −6.79 to −0.82 log cd.s.m
−2 , as well as the isolated rod PII at 2.07 log cd.s.m
−2 by minimizing the sum-of-squares merit function using the Excel Solver module (Microsoft).