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. 2016 May 5;44(Web Server issue):W395–W400. doi: 10.1093/nar/gkw395

Table 1. Loop-prediction performance of RCD+ and other state-of-the-art methods.

Nativea Modeling
HLPb Galaxy RCD+ HLP Galaxy Rosetta RCD+
Lengthc Std. PS2 1d 5 20 SS PS2 NGK 1 5 20
Median 0.6 0.6 0.5 0.3 0.3 0.9 1.1 0.4 0.5 0.4 0.4
8 Average 1.2 0.9 0.6 0.5 0.4 1.3 1.3 0.5 0.8 0.7 0.6
Sigma 1.5 0.7 0.3 0.3 0.2 1.5 1.0 0.3 1.0 1.0 0.8
#e 13 14 17 18 19 11 9 17 15 18 18
Median 0.6 1.4 0.6 0.4 0.4 0.9 1.6 0.8 0.6 0.6 0.5
12 Average 1.2 1.6 1.0 0.9 0.7 1.4 2.1 1.7 1.4 0.8 0.8
Sigma 1.2 1.3 1.7 1.0 1.0 1.4 1.7 1.8 1.6 0.9 0.9
#e 12 7 16 16 17 11 4 11 13 17 17

aSampling scenarios: (i) Native, the side-chains of the loop environment are kept, or (ii) Modeling, include the refinement of the loop environment side-chains.

bHLP, HLP-SS, Galaxy-PS2 and Rosetta-NGK Root Mean Squared Deviations (RMSDs) were taken from Supplementary Tables S1, S2, S4 and S5 of (8) and calculated considering the main-chain atoms N, Cα, C and O.

cNumber of residues of the loop.

dRMSD of the lowest Rosetta-energy loop predicted with RCD+ together with the best RMSD of the 5 and 20 loops of lowest Rosetta-energies.

eNumber of sub-angstrom cases.