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. 2014 Jun 18;53(28):4601–4611. doi: 10.1021/bi5005359

Figure 4.

Figure 4

(A and B) Single- and double-exponential fitting of the 520 nm ESA kinetic traces, respectively. The fit is convoluted with a 120 fs IRF (gray area). The residual of each fit is plotted above with the same y-axes for comparison of the single- and double-exponential fits.