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. 2021 Nov 10;120(23):5141–5157. doi: 10.1016/j.bpj.2021.11.010

Figure 3.

Figure 3

Ensemble refinement of WT apo-PhuS by ST, HDXer, and CD. (A) Plot of the trajectory-averaged RMSD (Å) of the Cα at each residue for the 5 μs conventional MD simulations of WT apo-PhuS (PDB: 4IMH) (black) and the combined six ST simulations of WT apo-PhuS (red). (B) The decision plot resulting from the reweighting of the combined ST ensemble to the target WT apo-PhuS HDX-MS data. The selected γ of 1 is displayed as a red dashed line. (C) Experimental CD spectra for apo-PhuS (red) and holo-PhuS (black). (D) Violin plots of the 11 significantly upweighted clusters ranked in order of average change in weight (log(Ωfi)). The tails represent the minimal and maximal weight in the cluster, the thick dashed lines are the mean weight, and the thin dashed lines bracket 50% of the population. The green dashed line represents the percent change in overall α-helicity (Δαh) observed between apo- and holo-PhuS unbiased MD simulations. The blue dots represent the Δαh between each of the 11 clusters and the holo-PhuS unbiased MD simulations, with the blue dashed-dot line representing the weighted average of the 11 blue dots. The red dotted line is the experimental Δαh measured by CD.