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The column definitions and tolerances are defined in the control file (see below).   
The column definitions and tolerances are defined in the control file (see below).   
==== Other input files  ====
Other files that can be included in an AutoStructure calculation inlcude:
*<sup>H</sup>N-H<sup>α</sup> J-couplings:&nbsp; used for initial secondary structrue anlysis
*slow exchanging NH list:&nbsp; used for initial secondary structrue anlysis
*dihedral angle constraints:&nbsp; used directly in CYANA/XPLOR&nbsp;structure calculations
*maunal distance constraints:&nbsp; used directly in CYANA/XPLOR&nbsp;structure calculations


=== Graphical User Interface  ===
=== Graphical User Interface  ===
AutoStructure features a GUI which is particularly useful for preparing the control file for and subsequent analysis of structure calulations.
The main page (Figure 1) features the following pull-down menus:
*File:&nbsp; manipulation of control file
*AutoStructure:&nbsp; starting an AutoStructure run and analysis of an output directory
*AutoQF(RPF):&nbsp; starting an RPF analysis and analysis of an RPF directory
*PDB&nbsp;Tools:&nbsp; tools for converting PDB coordinates to IUPAC format
*Misc Tools
==== Figure 1:&nbsp; AutoStructure main page ====


=== Control File<br>  ===
=== Control File<br>  ===

Revision as of 21:08, 7 November 2009

Introduction

Getting Started

Input Files

The following files are required to perform an AutoStructure run.

Protein sequence file

The sequence file must be in the following format:

1   @   MET    2   @   GLU    3   @   PHE    4   @   PRO    5   @   ASP
6   @   LEU    7   @   THR    8   @   VAL    9   @   GLU    10   @   ILE
....etc.

Here is an example sequence file.

Chemical shift assignment file

The chemical shift assignments for the protein must be in BMRB 2.1 format.  The header information is ignored.

AutoSructure does interpret the ambiguity code column.  This is important for denoting stereospecific assignments.

1       1       Met     HA      H       3.999   .       1
2       1       Met     HB2     H       2.011   .       2
3       1       Met     HB3     H       1.946   .       2
4       1       Met     HG2     H       2.368   .       2
5       1       Met     HG3     H       2.274   .       2
6       1       Met     CA      C       55.110  .       1
7       1       Met     CB      C       33.147  .       1
8       1       Met     CG      C       30.951  .       1
9       2       Glu     HA      H       4.548   .       1
....etc.

Here is an example bmrb file.

NOESY peak lists

AutoStructure can accept 3D and 4D NOESY peak lists.  In principle, any column formated peak list file can be read by the program; we typically use either Sparky or Xeasy formats. 

Here are example 15N-edited NOESY and 13C-edited NOESY peak lists.

The column definitions and tolerances are defined in the control file (see below). 

Other input files

Other files that can be included in an AutoStructure calculation inlcude:

  • HN-Hα J-couplings:  used for initial secondary structrue anlysis
  • slow exchanging NH list:  used for initial secondary structrue anlysis
  • dihedral angle constraints:  used directly in CYANA/XPLOR structure calculations
  • maunal distance constraints:  used directly in CYANA/XPLOR structure calculations

Graphical User Interface

AutoStructure features a GUI which is particularly useful for preparing the control file for and subsequent analysis of structure calulations.

The main page (Figure 1) features the following pull-down menus:

  • File:  manipulation of control file
  • AutoStructure:  starting an AutoStructure run and analysis of an output directory
  • AutoQF(RPF):  starting an RPF analysis and analysis of an RPF directory
  • PDB Tools:  tools for converting PDB coordinates to IUPAC format
  • Misc Tools

Figure 1:  AutoStructure main page

Control File

Staring a Calculation

The user can start a calculation from either the graphical user face or the command line. 

1. Launching a calculation from the GUI.

  • Under the Autostructure pull-down on the main page, choosing Start -> Calc opens the dialogue box below. 

AS startCalc.png

  • Launching calculations from the GUI uses is generally slow since only the processors on your own machine are used.  To speed up the calculations use the command line on a cluster.


2.  Launching a calculation from the command line.

  • Login in the a cluster.  At CABM we use AutoStructure version 2.2.1 on hummer.
  • A simple command line run can be started as follows:
/farm/software/AutoStructure/AutoStructure-2.2.1/bin/autostructure -c controlfile_CYANArun -o testCYANArun.out -v
  • Running the autostructure command gives the following options (like those avaliable in the GUI):
 AutoStructure/RPF Version 2.2.1 Copyright(C) 2007
     Center for Advanced Biotechnology and Medicine (CABM)
     Rutgers University

     Options:
         -c control_file      Required
         -o output_dir        Required
         -d                   For debug
         -h                   Help
         -m                   Exclude PCT-filter of Cycle1 for symmetry analysis
         -n                   Exclude CSI-based secondary structure analysis
         -i structure_file    inital fold for bootstrapping
         -j                   Include J-coupling constant data for angle constraint analysis (HYPER)
         -k float_number      Calibration coefficient
         -N                   Include NOE assignments in HYPER caluclation (under development)
         -q structure_file    AutoQF-Calculate the F and DP scores of the input structure_file (IUPAC naming)
         -r path              Restore from a prior outout_dir
         -R                   Include rotamer constraints in HYPER calculation (under development)
         -v                   Calculate the M score and average shifts

Files for Download

References

-- JimAramini - 07 Nov 2009