The AUDANA algorithm for automated protein 3D structure determination from NMR NOE data
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- Lee, W., Petit, C.M., Cornilescu, G. et al. J Biomol NMR (2016) 65: 51. doi:10.1007/s10858-016-0036-y
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We introduce AUDANA (Automated Database-Assisted NOE Assignment), an algorithm for determining three-dimensional structures of proteins from NMR data that automates the assignment of 3D-NOE spectra, generates distance constraints, and conducts iterative high temperature molecular dynamics and simulated annealing. The protein sequence, chemical shift assignments, and NOE spectra are the only required inputs. Distance constraints generated automatically from ambiguously assigned NOE peaks are validated during the structure calculation against information from an enlarged version of the freely available PACSY database that incorporates information on protein structures deposited in the Protein Data Bank (PDB). This approach yields robust sets of distance constraints and 3D structures. We evaluated the performance of AUDANA with input data for 14 proteins ranging in size from 6 to 25 kDa that had 27–98 % sequence identity to proteins in the database. In all cases, the automatically calculated 3D structures passed stringent validation tests. Structures were determined with and without database support. In 9/14 cases, database support improved the agreement with manually determined structures in the PDB and in 11/14 cases, database support lowered the r.m.s.d. of the family of 20 structural models.
Keywords3D structure determination Automated structure calculation NOE assignment PACSY database PONDEROSA Sequence-structure correlation
Three-dimensional structures of proteins provide important insights into their biological function. NMR spectroscopy is the sole approach for determining 3D structures of proteins in solution under near physiological conditions. In addition, NMR spectroscopy enables investigations of protein conformation and dynamics under different conditions. Whereas, structure determination from single-crystal X-ray diffraction has been largely automated, protein structure determination from NMR data still can require skilled manual intervention. This is particularly true for proteins that are large (>12 kDa), multimeric, or partially disordered. Most of the NMR-derived protein structures deposited in the Protein Data Bank (PDB) (Berman et al. 2009) represent monomeric proteins of fewer than 120 residues (Supplementary Fig. S1A). In addition, the number of NMR-derived structures is a small fraction of the total number of depositions (Supplementary Fig. S1B).
We have been developing an integrated approach to NMR-based protein structure determination that builds on NMRFAM-SPARKY (Lee et al. 2015), an updated and extended version of the highly popular Sparky program (Goddard and Kneller 2008). The Integrative NMR package (Lee et al. 2016) supports probabilistic methods for data interpretation (Bahrami et al. 2012; Lee et al. 2013) and automated structure determination from chemical shift assignments and NOE spectra (Lee et al. 2011). The structure determination package (PONDEROSA-C/S) (Lee et al. 2014) automates the identification of NOE cross peaks and the collection of torsion angle constraints. It also automates the data handling and format conversions required for use of the structure calculation modules of CYANA (Güntert 2004) and Xplor-NIH (Schwieters et al. 2003). The approach can flexibly incorporate data from other non-uniform sampling and reconstruction approaches (Dashti et al. 2015), such as ist@HMS (Hyberts et al. 2012) or NESTA-NMR (Sun et al. 2015).
Approaches have been introduced in recent years that take advantage of the growing number and variety of protein structures deposited in the Protein Data Bank (PDB) to assist in determining protein structures from NMR data. Shen and Bax (2007) introduced a method that employs SPARTA to refine fragment libraries used as input to Rosetta structure calculations (Shen et al. 2008). The CS-HM-Rosetta using 4D data has extended this approach to larger proteins (Thompson et al. 2012). The POMONA (protein alignments obtained by matching of NMR assignments) algorithm matches experimental chemical shifts to values predicted for the crystallographic database to generate templates for chemical shift-based Rosetta modeling. (Shen and Bax 2015). The CS23D (chemical shift to 3D structure) web server accepts chemical shifts and generates coordinates by means of homology modeling, chemical shift threading, or Rosetta-based shift-aided structure prediction (Wishart et al. 2008). Yet another bioinformatics approach combines sparse NMR data on a protein with distance restraints derived from evolutionary residue–residue couplings (Tang et al. 2015).
Initiation of a structure determination can be launched by two alternative methods: “AUDANA automation” or “PONDEROSA-X refinement”. The “AUDANA automation” optimizes user-supplied distance constraints, whereas the “PONDEROSA-X refinement” option runs AUDANA with automated NOESY assignments and torsion angle constraint optimization that automatically expands upper limits with elastic settings. By default, calculations are run on the NMRFAM-hosted Ponderosa Server. Users can run the software on their own hardware by installing the Ponderosa Server, the PACSY database, and the PACSY PDBSEQ_DB table expansion as described in Supplementary Table S1. AUDANA also can be launched directly from NMRFAM-SPARKY (Lee et al. 2015) by invoking “Calculation of 3D structure by PONDEROSA” (two-letter-code c3). The user then selects the NOESY spectra to be analyzed, and NOE cross peaks are identified automatically by the PONDEROSA algorithm. Alternatively, the user can submit NOE cross peaks chosen previously to the Ponderosa Web Server (http://ponderosa.nmrfam.wisc.edu/ponderosaweb.html). Structure calculations are carried out with the “PONDEROSA-X refinement” option, where “X” stands for Xplor-NIH annealing (Schwieters et al. 2003). Following the initial run, Ponderosa Client enables the user to add or modify constraints or change the calculation options.
AUDANA’s endurance scoring system consists of an endurance score, a supportive score, and a recycle bin. The endurance score for each distance constraint derived from NOESY data is determined initially by a statistical evaluation of the likelihood of its being correct. The endurance score is supplemented by the supportive score derived from finding similar structures in the database. The overall endurance score combines the supportive score with the endurance scores from NOESY data. The recycle bin is the place where violated distance constraints are temporarily stored. How they work together is described below.
AUDANA makes use of a queryable table “PDBSEQ_DB” (Supplementary Table S1) created by incorporating protein sequence data from the Protein Data Bank into the PACSY database. A total of 291,344 protein entries were included as of March 2016, and the resource is updated monthly. PDBSEQ_DB is available from the NMRFAM software download page (http://pine.nmrfam.wisc.edu/download_packages.html). By querying and aligning sequences from this table, AUDANA selects the three proteins with highest sequence homology to that of the target (Supplementary Fig. S2). Inter-proton distances determined from the structures of the homologous proteins are used to predict potential NOEs (Fig. 2); these predicted NOEs are filtered against the experimental NOESY data submitted by the user such that matches provide a supportive score for possible NOE assignments. However, if the sequence identity of the most similar protein is <20 %, no NOEs are predicted, and if it is >80 %, AUDANA uses only the structure of that single protein. The use of only one protein leads to a reduction in the supportive score and ensures that the structure of the target is not biased by that of the homolog because multiple sources of supportive score for the same constraint could be too high to be removed during the iterative structure calculation despite consistent violations.
During iterative structure calculation, AUDANA detects potential hydrogen bonds from NOE cross peak patterns for secondary structures and generates idealized H-bond constraints for the next cycle of calculation. After each calculation cycle, the H-bonds are reevaluated by measuring interatomic distances, and H-bond constraints that violate the structure are eliminated from use in the following cycle. Ponderosa Server automatically generates two Xplor-NIH constraint files from the H-bond constraints: the NOE constraint file, used to generate the NOE potential term (statically set to 30), and the HBDA constraint file, used for the HBDA potential term.
We tested AUDANA’s performance with data for 14 proteins (Supplementary Table S2). The Ponderosa Client program was used to import input data and run the calculations. To avoid biased cross validation, protein entries with identical sequences in the PACSY database were manually excluded from the sequence alignment process. Calculation options were set to “PONDEROSA-X refinement”, which runs AUDANA with torsion angle/rigid body dynamics and optimization by Xplor-NIH. We compared the lowest energy structure of each target to that of the first model deposited in the PDB (generally the representative structure with the lowest energy). All AUDANA calculated structures were very similar to those deposited in the PDB: the pairwise r.m.s.d. values for backbone atoms in ordered regions were less than 2 Å (mean r.m.s.d. of 1.41 ± 0.34 Å, Supplementary Table S2), and the superimposed structures were in close agreement (Supplementary Fig. S5). With these test proteins, AUDANA was instructed to select the best 20 out of 40 calculated structures at the phase III and IV. Targets considered difficult for automated NMR-based structure calculation, such as the symmetric homodimer NS1RBD (Supplementary Fig. S5E) and the 25 kDa protein mThTPase (Supplementary Fig. S5 N) were solved successfully with backbone r.m.s.d. values to the deposited structure of 1.32 and 1.58 Å, respectively.
For comparison, we used AUDANA to determine the structures of the same 14 proteins without database assistance (this is accomplished by unchecking the “Use PACSY DB for better NOE assignment” option in the Ponderosa Web Server). The results (Supplementary Table S2, rightmost column) show that 5 of the 14 data sets, including that for the homodimer (NS1RBD) and the 25 kDa protein (mThTPase), failed to converge or had backbone r.m.s.d. values to the deposited structures greater than 2.0 Å. Two of these proteins have large disordered regions (HR6470A and HR5537A). Five proteins (with closest sequence identities 94, 62, 38, 33, and 33 %) yielded lower backbone r.m.s.d. values to the deposited structures without database support; however, three of these had aromatic NOESY and RDC data in addition to the usual 13C-NOESY and 15N-NOESY data. This suggests that additional experimental data can circumvent the need for database support.
Structural assessment was conducted by the PSVS package (Bhattacharya et al. 2007). Ramachandran plot analysis results from both Procheck (Laskowski et al. 1996) and MolProbity (Chen et al. 2015) were satisfactory (Supplementary Table S4). The option of calculating the best 20 out of 40 calculated models led to acceptable convergence of the ensembles (ensemble backbone r.m.s.d. values between 0.28 and 0.80 Å; except for 2.76 Å for mThTPase, Supplementary Table S2). By using the more rigorous “constraints only for the final step” option, which calculates the best 20 out of 100 models, the ensemble backbone r.m.s.d. for mThTPase was reduced to 1.81 Å (Supplementary Fig. S6).
PONDEROSA-C/S offers two options in “constraints only for the final step”: (1) the traditional method of explicit water refinement followed by simulated annealing, and (2) concurrent implicit water solvation with EEFx (Effective Energy Function for Xplor-NIH) potential during simulated annealing (Tian et al. 2014). We found that option 2 was frequently better at generating energetically favorable structures than option 1.
Software availability AUDANA is available from http://pine.nmrfam.wisc.edu/download_packages.html. Web server, instruction, manuals and video tutorials can be found at http://ponderosa.nmrfam.wisc.edu. AUDANA has been incorporated into the PONDEROSA-C/S web service at NMRFAM, which is freely available to academic users. AUDANA is incorporated into the Integrative NMR platform (Lee et al. 2016), which requires the installation of NMRFAM-SPARKY, Ponderosa Analyzer, Ponderosa Client and PyMOL. The website provides instructions, installation scripts and video tutorials for their installation. AUDANA is also incorporated into the NMRFAM Virtual Machine (Lee et al. 2016) which contains pre-installed versions of all relevant software. The virtual machine (VM) can be run under a number of different virtualization software programs (VirtualBox and VMware among others) that support the Open Virtualization Format (.ovf,.ova). These virtualization programs are available for a wide variety of different popular host computers and operating systems (Windows, Mac OSX, Linux). A VM emulates a complete computer system. For example, the base operating system of the Integrative NMR VM is Ubuntu Mate 15.04 (64 bit Linux) (https://ubuntu-mate.org); the virtualization software allows this Linux VM to run natively on any host computer.
This work was supported by a grant (P41GM103399) from the Biomedical Technology Research Resources (BTRR) Program of the National Institute of General Medical Sciences (NIGMS), National Institutes of Health (NIH). We are grateful to Dr. Charles D. Schwieters for making Xplor-NIH sample scripts available. For the CASD-NMR targets, we thank the WeNMR project (European FP7 e-Infrastructure grant, contract no. 261572, www.wenmr.eu), supported by the European Grid Initiative (EGI) through the national GRID Initiatives of Belgium, France, Italy, Germany, the Netherlands, Poland, Portugal, Spain, UK, South Africa, Malaysia, Taiwan, the Latin America GRID infrastructure via the Gisela project, the International Desktop Grid Federation (IDGF) with its volunteers, and the US Open Science Grid (OSG).
|Funder Name||Grant Number||Funding Note|
|National Institute of General Medical Sciences|
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