| Literature DB >> 24397429 |
Adrien B Larsen1, Jeffrey R Wagner, Abhinandan Jain, Nagarajan Vaidehi.
Abstract
A longstanding challenge in using computational methods for protein structure prediction is the refinement of low-resolution structural models derived from comparative modeling methods into highly accurate atomistic models useful for detailed structural studies. Previously, we have developed and demonstrated the utility of the internal coordinate molecular dynamics (MD) technique, generalized Newton-Euler inverse mass operator (GNEIMO), for refinement of small proteins. Using GNEIMO, the high-frequency degrees of freedom are frozen and the protein is modeled as a collection of rigid clusters connected by torsional hinges. This physical model allows larger integration time steps and focuses the conformational search in the low frequency torsional degrees of freedom. Here, we have applied GNEIMO with temperature replica exchange to refine low-resolution protein models of 30 proteins taken from the continuous assessment of structure prediction (CASP) competition. We have shown that GNEIMO torsional MD method leads to refinement of up to 1.3 Å in the root-mean-square deviation in coordinates for 30 CASP target proteins without using any experimental data as restraints in performing the GNEIMO simulations. This is in contrast with the unconstrained all-atom Cartesian MD method performed under the same conditions, where refinement requires the use of restraints during the simulations.Entities:
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Year: 2014 PMID: 24397429 PMCID: PMC3985798 DOI: 10.1021/ci400484c
Source DB: PubMed Journal: J Chem Inf Model ISSN: 1549-9596 Impact factor: 4.956
Extent of Refinement in the GDT and TM Scores from GNEIMO Compared with the Best Structure Submitted in CASP for Each Targeta
| TR Decoys, All C-alpha | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| GDT_TS | TM-Score | RMSD | |||||||
| target | start | best GNEIMO | best CASP | start | best GNEIMO | best CASP | start | best GNEIMO | best CASP |
| 429 | 31.5 | 45.7 | 39.8 | 0.46 | 0.59 | 0.53 | 6.82 | 5.76 | 6.62 |
| 435 | 80.2 | 87.9 | 83.4 | 0.86 | 0.91 | 0.89 | 2.14 | 1.65 | 1.88 |
| 453 | 86.6 | 91.5 | 86.6 | 0.87 | 0.92 | 0.88 | 1.51 | 1.10 | 1.48 |
| 454 | 58.5 | 71.0 | 60.2 | 0.79 | 0.87 | 0.81 | 3.26 | 2.47 | 3.09 |
| 461 | 89.4 | 91.2 | 90.4 | 0.93 | 0.94 | 0.94 | 1.63 | 1.55 | 1.60 |
| 462 | 63.8 | 67.1 | 69.1 | 0.80 | 0.81 | 0.83 | 2.55 | 2.55 | 2.28 |
| 464 | 75.4 | 83.3 | 81.2 | 0.76 | 0.81 | 0.82 | 2.77 | 2.45 | 2.28 |
| 469 | 76.6 | 80.3 | 89.3 | 0.74 | 0.79 | 0.85 | 2.13 | 1.89 | 1.68 |
| 476 | 36.5 | 45.8 | 42.5 | 0.42 | 0.50 | 0.47 | 6.92 | 6.31 | 5.42 |
| 488 | 85.3 | 86.8 | 90.5 | 0.88 | 0.89 | 0.92 | 2.13 | 1.91 | 1.57 |
| 517 | 68.5 | 72.8 | 69.4 | 0.77 | 0.80 | 0.78 | 4.60 | 3.59 | 3.95 |
| 530 | 82.4 | 90.7 | 88.5 | 0.84 | 0.90 | 0.88 | 2.00 | 1.33 | 1.63 |
| 557 | 63.4 | 68.0 | 66.6 | 0.73 | 0.76 | 0.78 | 4.10 | 3.37 | 3.30 |
| 568 | 50.8 | 53.9 | 56.2 | 0.55 | 0.57 | 0.60 | 6.26 | 5.60 | 4.26 |
| 569 | 68.4 | 72.2 | 77.8 | 0.71 | 0.73 | 0.81 | 3.05 | 2.94 | 1.98 |
| 574 | 57.3 | 66.4 | 58.6 | 0.64 | 0.72 | 0.65 | 3.52 | 2.90 | 3.37 |
| 576 | 61.3 | 61.3 | 66.4 | 0.72 | 0.72 | 0.76 | 6.67 | 6.67 | 3.86 |
| 592 | 89.8 | 93.5 | 93.4 | 0.92 | 0.94 | 0.95 | 1.22 | 1.09 | 0.95 |
| 594 | 85.3 | 85.5 | 85.8 | 0.90 | 0.91 | 0.91 | 1.83 | 1.62 | 1.64 |
| 606 | 67.1 | 67.1 | 75.9 | 0.73 | 0.73 | 0.81 | 4.87 | 3.95 | 2.91 |
| 614 | 71.9 | 71.9 | 80.2 | 0.76 | 0.76 | 0.84 | 5.36 | 4.41 | 2.78 |
| 622 | 66.7 | 66.7 | 73.5 | 0.74 | 0.74 | 0.78 | 6.54 | 6.17 | 3.25 |
| 624 | 50.0 | 59.3 | 63.4 | 0.49 | 0.58 | 0.63 | 5.21 | 3.95 | 3.86 |
| avg score | 68.1 | 73.0 | 73.4 | 0.74 | 0.78 | 0.79 | 3.79 | 3.27 | 2.85 |
| avg improvement | 4.9 | 5.3 | 0.04 | 0.05 | 0.52 | 0.93 | |||
The third column in each block shows the scores for the best structure submitted to CASP. Note that the best CASP structure came from different groups. The RMSD deviations have been calculated for the Cα atoms in angstroms.
Extent of Refinement in the GDT and the TM Score of the Best Structure from the GNEIMO-REXMD Trajectories for the CASP Structure Prediction Targetsa
| TO MODELER Decoys, All C-alpha | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| GDT_TS | TM-Score | RMSD | |||||||
| Target | start | best GNEIMO | best CASP | start | best GNEIMO | best CASP | start | best GNEIMO | best CASP |
| T0387 | 85.7 | 89.3 | 95.5 | 0.88 | 0.90 | 0.94 | 1.95 | 1.43 | 1.01 |
| T0453 | 80.3 | 83.0 | 87.1 | 0.82 | 0.84 | 0.89 | 3.75 | 1.85 | 1.47 |
| T0469 | 82.0 | 86.5 | 73.4 | 0.79 | 0.83 | 0.74 | 1.93 | 1.88 | 2.47 |
| T0472 | 89.5 | 89.7 | 61.8 | 0.93 | 0.93 | 0.76 | 1.21 | 1.06 | 2.68 |
| T0488 | 71.8 | 75.3 | 86.0 | 0.75 | 0.79 | 0.87 | 4.60 | 3.54 | 1.97 |
| T0492 | 82.3 | 92.7 | 85.8 | 0.82 | 0.91 | 0.87 | 1.67 | 1.16 | 1.70 |
| T0554 | 67.1 | 73.7 | 32.3 | 0.80 | 0.84 | 0.44 | 3.40 | 2.65 | 8.31 |
The RMSD deviations have been calculated for the Cα atoms in angstroms.
Figure 1(A–D) Refinement of CASP targets with different types of secondary structure as shown in the figures and corresponding distance-to-native map. The distance to native map shows how far each residue is corresponding to the native structure. (1A) Example of refinement of loop structure; (1B) refinement of β-sheet packing; (1C) packing of α-helices; (1D) β-sheet growth; (1E) example of a structure that was not refined by GNEIMO.
Figure 2Population distribution of the ensemble generated from the GNEIMO simulations compared to the Cartesian simulations for various refinement CASP targets. The dotted line is the GDT_TS score for the starting decoy.
Figure 3Potential energies of the conformations generated in the GNEIMO-REXMD simulation trajectories calculated using (a) AMBER99SB all atom forcefield and (b) Rosetta energy function.