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. 2021 Apr 12;4:453. doi: 10.1038/s42003-021-01986-6

Fig. 3. Force-loading rate dependence for the vWF-vWbp-ClfA ternary interaction follows Bell–Evans dynamics.

Fig. 3

Left: dynamic force spectroscopy plot of rupture force vs loading rate (n = 2992 curves from 3 cells, for individual data from 6 cells see Supplementary Fig. 2). The dotted line shows the extrapolated Bell–Evans fit through the most probable (mean) rupture forces and loading rates for five log-equispaced loading rate bins shown as solid circles. Error bars are the standard deviations. Right: corresponding histograms of the plot shown on the left.