2010 AMBER Tutorial with Biotin and Streptavidin

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In this tutorial, we will learn how to run a molecular dynamics simulation of a protein-ligand complex. We will then post-process that simulation by calculating structural fluctuations (with RMSD) and free energies of binding (MM-GBSA).

Biotin Notes

Biotin is also called vitamin H. And it takes part in multiple processes inside the cell. It's a B-complex vitamin (coenzyme) that's involved in gluconeogenesis, citric acid cycle, and various carboxylation reactions.

Streptavidin Notes

Download PDB Here and view it's details Here. Streptavidin has an incredibly strong affinity for biotin; the dissociation constant for the streptavidin-biotin complex is on the order of femtomolar.

.... ....

What is AMBER?

Amber - Assisted Model Building with Energy Refinement - is a suite of about 50 programs that can be used to simulate, study and analyze macromolecular systems such as proteins dissolved in water at physiological conditions. Amber10, the current version (Amber11 soon to be released) of Amber, is extremely advanced, powerful and fast. PMEMD, particle mesh Ewald MD (boundary condition treatment / parallelized code) can churn out 314 ps/day of data for the system dihydrofolate reductase (159 residue protein) in TIP3P water (23,558 total atoms). However, because PMEMD lacks the ability to restrain the atoms we need properly, we will be using SANDER to perform most of our simulations.


The Amber 10 Manual is the primary resource when trying to learn what variables and keywords mean and what they do. Using Adobe Acrobat to view the file, you can simply search the document for keywords, which saves much time.

Keywords for preparatory programs:

LEaP: creates or modifies systems in Amber. It consists of the functions of prep, link, edit, and parm.

ANTECHAMBER: the main Antechamber suite program that helps prepare input files for nucleic acids and proteins for LEaP.

Keywords for simulating programs:

SANDER: according to the Amber 10 manual, it is 'a basic energy minimizer and molecular dynamics program. This program relaxes the structure by iteratively moving the atoms down the energy gradient until a sufficiently low average gradient is obtained. The molecular dynamics portion generates configurations of the system by integrating Newtonian equations of motion. MD will sample more configurational space than minimization, and will allow the structure to cross over small potential energy barriers. Configurations may be saved at regular intervals during the simulation for later analysis, and basic free energy calculations using thermodynamic integration may be performed. More elaborate conformational searching and modeling MD studies can also be carried out using the SANDER module. This allows a variety of constraints to be added to the basic force field, and has been designed especially for the types of calculations involved in NMR structure refinement'.

PMEMD: verison of SANDER that allows parallel scaling and optimized speed.

There is a mailing list you could sign-up for, as an additional resource.

Unix tips

This is specific to our cluster (seawulf) and desktop (mathlab) environments. See Activating your Seawulf Account for details of sw short cut.

Download Files from SeaWulf to Herbie:

ssh compute.mathlab.sunysb.edu

Login in to Herbie

mkdir sw_dir

make a directory "sw_dir" for which to download files and be organized

cd to sw_dir so when you scp files or directories back to Herbie, it copies them to a specific directory - "sw_dir"

cd sw_dir
scp -r sw:/location_of_files_or_directory/ .

Safely Copy, Recursively, /location_of_files_or_directory/


include these lines before mpirun command to know which nodes mpi is running on

echo "Queue is giving this nodes:"
echo "MPI is running on:"
mpirun -n 8 hostname

Structure Preparation

To begin with, create the directories in seawulf you will work in, using the commands here:

mkdir AMBER_Tutorial
cd AMBER_Tutorial
mkdir 001.CHIMERA.MOL.PREP  
mkdir 002.TLEAP  
mkdir 003.SANDER 
mkdir 004.ptraj

Copy the commands above to your terminal and hit enter one at a time.

Open Chimera, choose File - Fetch by ID, then type in "1df8". Now you will see your protein and ligand in Chimera.

1. It is a dimer, but you need only a monomer.

  • Click Select - chain - B, you would see chain B is highlighted.
  • Then click Action - Atoms/Bonds - delete.

Now only a receptor, a ligand and several water molecules are left.

2. Now you need to separate the ligand and receptor.

  • First, Select - residue - HOH, then delete it.
  • File - Save PDB, save this pdb as "1df8.rec_lig.pdb", then Select - residue - BTN, delete it. Save PDB as "1df8.rec.noh.pdb."
  • Now you have a receptor pdb file, place it in your "001.CHIMERA.MOL.PREP" directory by performing the following:
    • put files on a machine that is a portal to seawulf (i.e. silver, herbie or ringo). If user is on a MATHLAB machine then files are acessible from silver or herbie.
    • scp files sw:path
      • Note that is only applies to AMS536 (or Rizzo lab rotation) students and is specific for our computer setup.
  • Second, open the 1df8.rec_lig.pdb, select the receptor and delete it (Tips: you can invert your selection.)
    • Then Tools - structure editing - Add H, press OK.
    • Then Tools - structure editing - Add Charge, press OK. select AM1-BCC charge model.
    • File - Save mol2, save it as "1df8.lig.mol2".

Note that this mol2 file would cause errors later in leap, because of its numbering. You need to modify it manually. Simply you can copy this file from "/nfs/user03/pholden/AMBER_Tutorial/001.CHIMERA.MOL.PREP/1df8.lig.mol2" on seawulf, and compare it with yours to see what should be modified. Also, place it in your "001.CHIMERA.MOL.PREP" directory. Note that there are four residues (22, 27, 40, and 57) that have two possible conformers, when tleap builds your parm and crd files only the first occurrence of each atom is kept. See section below and leap output.


Class please add in a Tleap section here.

Class I've gotten a section started please improve this section. Thanks.

describe our protocol and give example input files.

First, create directory called ~/AMBER_Tutorial/002.TLEAP and go into that dir:

mkdir ~/AMBER_Tutorial/002.TLEAP
cd ~/AMBER_Tutorial/002.TLEAP

Next we will write the following files that you will need to input files for LEAP in order to create your parameter/topology files and your coordinate files

cat << EOF > tleap.lig.in
set default PBradii mbondi2
source leaprc.ff99SB
loadamberparams rizzo_amber7.ionparms/parm.e16.dat
loadoff rizzo_amber7.ionparms/ions.lib
loadamberparams rizzo_amber7.ionparms/ions.frcmod
source leaprc.gaff
loadamberparams rizzo_amber7.ionparms/gaff.dat.rizzo
loadamberparams 1df8.lig.ante.frcmod
loadamberprep 1df8.lig.ante.prep
lig = loadpdb 1df8.lig.ante.pdb
saveamberparm lig 1df8.lig.gas.leap.parm 1df8.lig.gas.leap.crd
solvateBox lig TIP3PBOX 10.0
saveamberparm lig 1df8.lig.wat.leap.parm 1df8.lig.wat.leap.crd
charge lig
cat << EOF > tleap.rec.in
set default PBradii mbondi2
source leaprc.ff99SB
loadamberparams rizzo_amber7.ionparms/parm.e16.dat
loadoff rizzo_amber7.ionparms/ions.lib
loadamberparams rizzo_amber7.ionparms/ions.frcmod
REC = loadpdb ../001.CHIMERA.MOL.PREP/1df8.rec.noh.pdb

saveamberparm REC 1df8.rec.gas.leap.parm 1df8.rec.gas.leap.crd
solvateBox REC TIP3PBOX 10.0
saveamberparm REC 1df8.rec.wat.leap.parm 1df8.rec.wat.leap.crd
charge REC
cat << EOF > tleap.com.in
set default PBradii mbondi2
source leaprc.ff99SB
loadamberparams rizzo_amber7.ionparms/parm.e16.dat
loadoff rizzo_amber7.ionparms/ions.lib
loadamberparams rizzo_amber7.ionparms/ions.frcmod
source leaprc.gaff
loadamberparams rizzo_amber7.ionparms/gaff.dat.rizzo
REC = loadpdb ../001.CHIMERA.MOL.PREP/1df8.rec.noh.pdb

loadamberparams 1df8.lig.ante.frcmod
loadamberprep 1df8.lig.ante.prep
LIG = loadpdb 1df8.lig.ante.pdb
COM = combine {REC LIG}
saveamberparm COM 1df8.com.gas.leap.parm 1df8.com.gas.leap.crd
solvateBox COM TIP3PBOX 10.0
saveamberparm COM 1df8.com.wat.leap.parm 1df8.com.wat.leap.crd
charge COM

Note the rizzo_amber7.ionparms/*.dat are modified parameter files.

The following is an example csh script the

#! bin/csh

set workdir = "~/AMBER_Tutorial/002.TLEAP"
cd $workdir


antechamber -i ../001.CHIMERA.MOL.PREP/1df8.lig.mol2 -fi mol2  -o 1df8.lig.ante.pdb  -fo pdb
antechamber -i ../001.CHIMERA.MOL.PREP/1df8.lig.mol2 -fi mol2  -o 1df8.lig.ante.prep -fo prepi
parmchk -i 1df8.lig.ante.prep -f  prepi -o 1df8.lig.ante.frcmod
tleap -s -f tleap.lig.in > tleap.lig.out
tleap -s -f tleap.rec.in > tleap.rec.out
tleap -s -f tleap.com.in > tleap.com.out

ambpdb -p   1df8.com.gas.leap.parm -tit "pdb" <1df8.com.gas.leap.crd > 1df8.com.gas.leap.pdb


To parameterize your ligands the following is done.

antechamber is run first to create a prepi file. Then parmchk is run to create a frcmod file. This files are need be for running leap. You can see if you look in the tleap.com.in and tleap.lig.in the frcmod is loaded:

loadamberparams 1df8.lig.ante.frcmod

It is a good idea to open all these files with your favorite text editor (eg. vim).

consult the amber manual to see what each of this contains.

Class I think that you should describe the output here. thanks.

TLEAP Generating Data

open 002.tleap and the file should look like:

" ============================================================================
" Netrw Directory Listing                                        (netrw v125)
"   /nfs/user03/username/1DF8_setup/AMBER_tutorial/002.TLEAP
"   Sorted by      name
"   Sort sequence: [\/]$,\.h$,\.c$,\.cpp$,*,\.o$,\.obj$,\.info$,\.swp$,\.bak$,\~$
"   Quick Help: <F1>:help  -:go up dir  D:delete  R:rename  s:sort-by  x:exec
" ============================================================================

now do csh to create the coordinate and parm files

Minimization and equilibration

In order to adjust our structures to the force field and remove any model building artifacts, we first perform a several-step equilibration protocol. Several iterations of minimization and molecular dynamics will be preformed with decreasing restraints.

The first step: Relaxing the experimental or silico structure

01mi.in: equilibration
  imin = 1, maxcyc = 1000, ntmin = 2,
  ntx = 1, ntc = 1, ntf = 1,
  ntb = 1, ntp = 0,
  ntwx = 1000, ntwe = 0, ntpr = 1000,
  scee = 1.2, cut = 8.0,
  ntr = 1,
  restraintmask = ':1-119 & !@H=',            

The MD run should be set up:

cat << EOF > 10md.in
10md.in: production (500000 = 1ns)
   imin = 0, ntx = 5, irest = 1, nstlim = 500000,
   temp0 = 298.15, tempi = 298.15, ig = 71287,
   ntc = 2, ntf = 1, ntt = 1, dt = 0.002,
   ntb = 2, ntp = 1, tautp = 1.0, taup = 1.0,
   ntwx = 500, ntwe = 0, ntwr = 500, ntpr = 500,
   scee = 1.2, cut = 8.0, iwrap = 1,
   ntr = 1, nscm = 100,
   restraintmask = ':1-118@CA,C,N', restraint_wt = 0.1,

  • &cntrl -> Tells SANDER that what follows are control variables.
  • imin=1 -> Perform Minimization
  • maxcyc=1000 -> Perform 1000 Minimization Steps
  • ntmin=2 -> Steepest Descent Method of Minimization
  • ntx=1 -> Initial Coordinates Lack Velocity - it's a restart file (See VMD)
  • ntc=1 -> "SHAKE" Posititional Restraints OFF (Default)
  • ntf=1 -> Calculate All types of Forces (bonds, angles, dihedrals, non-bonded)
  • ntb=1 -> Constant Volume Boundary Periodicity
  • ntp=0 -> No Pressure Regulation
  • ntwx=1000 -> Print Coordinates Frequency
  • ntwe=0 -> Print Energy to "mden" Frequency
  • ntpr=1000 -> Print Readable Energy Information to "mdout" and "mdinfo"
  • scee' -> 1-4 Coulombic Forces are Divided (Default=1.2)
  • cut=8.0 -> Coulombic Force Cutoff distance in Angstroms
  • restraintmask = ':1-119 & !@H=', -> restraint the residues matching the mask':1-119 & !@H='. Here, we're restraining residues 1 through 119 and everything that isn't hydrogen. Essentially, onlt Hydrogen atoms move free of restraint.
  • restraint_wt=5.0 is the Force Constant assigned to the restrained atoms. Each atom "sits" in a potential-energy well characterized by a "5.0" kcal/mol wall.
  • / is used to the machine to stop the job when it's done.

Class add in exactly what your equilibration was.

When your simulations have finished, you ought to check the stability and realism of results. Use the script E_asis to analyze the the mdout files. This ought to also be used to check the validity and stability of your production runs.

Download E_asis onto your local machine (the one you're using right now). Once saved onto local machine, transfer it to you working directory on Herbie, Seawulf, etc. Follow usual protocols to do this. This script will extract the energy, temperature, pressure and volume (and averages thereof) from the mdout file. To execute, do the following (it may be a good idea to make a separate directory just for this analysis, as many files are created):

chmod +x E_asis

./E_asis Filename.out

Filenames, as per this tutorial ought to be 01min, 02md, 03md, etc. To analyze the whole equilibration experiment (i.e. 01min to 09md), the following may work. Please check the results to be sure it worked properly. There are various ways to coordinate the analysis of these output files..

./E_asis *.out

Production Simulation

(Class please describe your production run simulations...)

A Production simulation is the ultimate simulation to be performed. Once the structure is built (See tLeap section), minimized and equilibrated (See Minimization and equilibration section) and only essential restraints retained, production dynamics produce the data used to answer the scientific question at hand. The previous steps were just preparatory.

The script used to instruct the supercomputer how to perform the dynamics:


#! bin/csh
set workdir = "/nfs/user03/Your User Name/AMBER_Tutorial/003.SANDER"
cd ${workdir}
set coor = "../002.TLEAP/1df8.com.wat.leap.crd"
set topo = "../002.TLEAP/1df8.com.wat.leap.parm"
cat << EOFQSUB > temp.qsub.csh
#! /bin/tcsh
#PBS -l nodes=4:ppn=2
#PBS -l walltime=720:00:00
#PBS -o zzz.qsub.out
#PBS -e zzz.qsub.err
cd ${workdir}
cat \$PBS_NODEFILE | sort | uniq
cat \$PBS_NODEFILE | sort | uniq > mpd.nodes
#I have Deleted The cat'ing of input files that appeared in "run.sander.MPI.csh"
#I have Deleted the "mpiexec" aka "mpirun" for jobs 1 through 9
mpirun -n 8 sander.MPI -O -i 10md.in -o 10md.out -p ${topo} -c 09md.rst -ref 05mi.rst -x 10md.trj -inf 10md.info -r 10md.rst
mpirun -n 8 sander.MPI -O -i 11md.in -o 11md.out -p ${topo} -c 10md.rst -ref 05mi.rst -x 11md.trj -inf 11md.info -r 11md.rst
chmod +x temp.qsub.csh
qsub temp.qsub.csh

The important instructions are the 18th and 19th lines - mpirun.

mpirun - Instructs SeaWulf (SW) to use an mpi regime.

-n - Denotes number of processors (Here 8)

sander.MPI - Is the actual MPI code to be run. This is the heart of the whole course. The text after this and on this line will be instructions for sander.

-O Overwrite previous output files with the new ones (to be produced by this job). This is useful in that if you have to run this script more than once, then something must have gone wrong. Thus, this will simply overwrite the files that are erroneous anyways. Don't use this if you really know what your doing and have a reasonable reason for doing so.

-i Points sander to the input file (10md.in then 11md.in).

-o Instructs sander to write the output file (10md.out then 11md.out), which contains the energies written by sander during dynamics. The various variables within the input file will determine the nature of the output: How frequently are the energies printed? How detailed is the information? What types of energies are being printed?

-p Points sander to the topology (aka parameter file). See Amber10 manual if you don't know what this is.

-c Points sander to the coordinates (corresponding to the topology file from above) for which you want the production dynamics to begin from. In this case, we're starting with the final (snapshot - single frame) frame from the previous (equilibration) run, 9md.rst. The .rst at the end of a file means "restart". "restart" files are single frames. They can contain subtle information in addition to simply the number of atoms in the file (first line) and the x, y and z coordinates for each atom (which is why you need the topology file to give those x,y,z's meaning - what atom has what coordinates) so check the Amber10 manual if you're curious.

-ref Specifies for sander which file you would like the restraints (if not using restraints, then -ref is not used) to be centered on. Asking Professor Rizzo to explain this flag is a good idea, after reading the Amber10 manual (don't waste his time), of course, if it is critical to your work. If not: the reference is a snapshot-set of coordinates which you have carefully chosen to represent the "ideal" structure you would like the dynamics (sander) to use as a "reference"; using the restrain_wt option in the input file, you're telling sander how much like the reference structure you want your dynamical system to be. The restraint_wt option acts like a spring, where harmonically the reference coordinates and coordinates of the dynamical system are "psuedo-connected." Thus, it is imperative that the reference structure be realistic (say the coordinates of the crystal structure) and be the same system (i.e. same number of atoms).

-x Instructs sander to print the trajectory (position of each atom along with its velocity) every ntwx steps. This is the "Big" file. When your simulation is complete, zip the trajectories:

gzip 10md.trj

gzip 11md.trj

The trajectories are, in my opinion, the most important component of a MD experiment. So, read the Amber10 Manual. You could notice that ptraj uses the trajectory files to perform the bulk of the data analysis like RMSD, H-bonding evolution, radius of gyration, pi-stacking, etc., etc.

-info Gives the results of the interactions between the supercomputer and sander: How did the calculation proceed? Did everything work properly? Did the simulation run to completion? This flag can be useful in debugging failed jobs....hk...

-r Instructs sander to write a restart file. The frequency this is done is specified is ntwr in the 10md.in / 11md.in files. Usually ntwr=500. A restart file will be written at the end of the simulation - the final snapshot of the simulation will be the restart file if and when the simulation has run successfully to completion. During the simulation, however, this file is continuously re-written as a fail-safe - say the supercomputer crashes during your 10ns simulation, which has been running for 3 weeks. Well, the restart file is printed every ntwr steps so you could, as the name of the flag implies, simply restart the simulation (with minor modification to the input file and above runsander.csh script) from the last snapshot before the crash.

ptraj - Analyzing Your Data

ptraj is an analysis program included in the AMBER suite (AMBERtools) designed in part by Dr. Thomas Cheatham. See this website.

This page contains a brief list of ptraj functions and their syntax. Commands can be combined with most combinations of other functions to suit the need.

A useful and recommended program - merely a text file with functional syntax - to write is:


ptraj <filename.parm> <ptraj.1.in> > <ptraj.1.out>

(When writing the above, one depressed 'Enter' on the keyboard, which is 'recorded' by vim. So, when the file is executed, it would be like hitting 'Enter' if you were entering the commands by hand in the shell.

  • Change filename.parm to 1df8.com.gas.leap.parm

#!/bin/csh -> will be in nearly all of the programs you will write - bash and tcsh are other scripting languages. It tells the shell to treat the contents of this here file as if the contents were being typed in the shell by hand.

ptraj -> has been aliased in your .cshrc file and will initialize ptraj once read by the machine.

filename.parm -> is the .parm file you would like to specify.

ptraj_input_filename.1.in -> is the set of instruction you want ptraj to read and perform, in an input file (This would be "ptraj.concatenate.strip.trj" in the coming examples).

exit -> will exit from ptraj when the ptraj_input_filename.1.in has completed its instruction(s).

Executing it:

Herbie:~> csh RUNTRAJ

1. Combine Production Trajectories while Stripping the Water Molecules


 trajin ../003.SANDER/10md.trj 1 1000 1
  • trajin -> tells ptraj to "read-in" the file which comes after it
  • ../003.SANDER/10md.trj -> is the file to be "read-in"
  • 1 1000 1 -> tells ptraj to use the first to the 1000th snapshot of the trajectory. The third number, "1", is telling ptraj to read-in every frame. If this last number were "2", then ptraj would read-in every-other snapshot, "10" would be every 10th snapshot and so on.
trajin ../003.SANDER/11md.trj 1 1000 1
  • This will do the exact same as the first trajin cmd (command), except now we're analyzing a different trajectory - 11md.trj.
trajout 1df8.trj.strip nobox
  • trajout -> tells ptraj to write a new trajectory file, combining the two trajectories - 10md.trj and 11md.trj - from trajin.
  • 1df8.trj.strip -> is the name of the new trajectory to be made by trajout.
  • nobox -> is essentially a house-keeping cmd, where the periodic box information will just be neglected. Unless using CHARMM files, this ought to not be an issue.
strip :WAT
  • strip -> instructs ptraj to disappear those objects named "WAT" ':WAT
  • So you're left with a file "ptraj.concatenate.strip.trj" with the following in it:
trajin ../003.SANDER/10md.trj 1 1000 1
trajin ../003.SANDER/11md.trj 1 1000 1
trajout 1df8.trj.strip nobox
strip :WAT


RMSD - root mean-square distance - can be used to measure the distance an object moves relative to a reference object. For example, one could use an RMSD analysis to measure the movement of the alpha-carbon atoms in the active site of a protein, using the experimental structure as the reference structure (ptraj will measure the RMSD between each object specified in the ptraj script - see below) where ptraj will by default fit the two structures, aligning them as much as possible. nofit is used to turn this function off.


 trajin 1df8.trj.strip 1 2000 1
 trajout 1df8.com.trj.stripfit
 reference 1df8.com.gas.leap.crd
  • reference -> tells ptraj that you want to specify a reference file - snapshot - for which to compare your trajectory (file with many snapshots) to.
  • 1df8.com.gas.leap.crd -> is the reference file. This file is very important and you ought to be thoughtful about your selection of this file. Usually, when possible, one wants to use the experimental structure as the reference. Referencing the experimental structure 'usually' provides the most informative results. But, if done thoughtfully, a non-experimental reference could be informative, too...
 rms reference out 1df8.rmsd.CA.txt :1-118@CA
  • rms -> tells ptraj you want to perform an rms analysis
  • reference -> tells traj to use the reference file, specified in the previous line
  • out -> tells ptraj to create a temporary file out for which to store calculations during the analysis
  • 1df8.rmsd.CA.txt -> is the name of the file with the RMSD analysis results. This is the file you will use with your plotting program..
  • :1-118@CA -> tells ptraj to analyze the RMSD of the alpha-carbon atoms CA residues 1-118.

So when you're done, you're left with:

trajin 1df8.trj.strip 1 2000 1
trajout 1df8.com.trj.stripfit
reference 1df8.com.gas.leap.crd
rms reference out 1df8.rmsd.CA.txt :1-118@CA

4. Keep Only Streptavidin from 1df8.com.trj.stripfit


trajin 1df8.com.trj.stripfit 1 2000 1
trajout 1df8.rec.trj.stripfit
strip :119
  • We've just stripped residue 119 (Biotin) from the 1df8.com.trj.stripfit file, which we've previously stripped of water

5. Keep Only Biotin from 1df8.com.trj.stripfit


trajin 1df8.com.trj.stripfit 1 2000 1
trajout df8.lig.trj.stripfit
strip :1-118
  • Strip everything, keeping only the protein, Streptavidin

Also, you can write a csh file to go through the procedure above. Make a file analy.1.csh in your AMBER_tutorial directory as follows:

#! /bin/tcsh

mkdir 004.PTRAJ
cd ./004.PTRAJ

cat << EOF > ptraj.1.in
trajin ../003.SANDER/10md.trj 1 1000 1
trajin ../003.SANDER/11md.trj 1 1000 1
trajout 1df8.trj.strip nobox
strip :WAT

ptraj ../002.TLEAP/1df8.com.wat.leap.parm ptraj.1.in >ptraj.1.log

cat << EOF > ptraj.2.in
trajin 1df8.trj.strip
trajout 1df8.com.trj.stripfit
reference ../002.TLEAP/1df8.com.gas.leap.crd
rms reference out 1df8.rmsd.CA.txt :1-118@CA

ptraj ../002.TLEAP/1df8.com.gas.leap.parm ptraj.2.in >ptraj.2.log

cat << EOF > ptraj.3.in
trajin 1df8.com.trj.stripfit
reference ../002.TLEAP/1df8.com.gas.leap.crd
rms reference out 1df8.lig.rmsd.txt :119@C*,N*,O*,S* nofit

ptraj ../002.TLEAP/1df8.com.gas.leap.parm ptraj.3.in >ptraj.3.log 

cat << EOF > ptraj.4.in
trajin 1df8.com.trj.stripfit
trajout 1df8.rec.trj.stripfit
strip :119

cat <<EOF > ptraj.5.in 
trajin 1df8.com.trj.stripfit
trajout 1df8.lig.trj.stripfit
strip :1-118

ptraj ../002.TLEAP/1df8.com.gas.leap.parm ptraj.4.in >ptraj.4.log
ptraj ../002.TLEAP/1df8.com.gas.leap.parm ptraj.5.in >ptraj.5.log  

cd .. 

Then use "csh" command to execute the file analy.1.in in your AMBER_tutorial directory.

Hydrogen bond distance

Before using ptraj to measure the H-bond distance, it's better to know which atoms we want to put in the ptraj script. VMD can automatically draws these H-bonds. First, select the ligand and residues around the ligand. Second, change the Drawing Method to HBonds.

After we know the atom name, we use distance command to measure the distance between two atoms. Here is the sample script

ptraj ../002.TLEAP/1df8.com.gas.leap.parm << EOF
trajin ../004.PTRAJ/1df8.com.trj.stripfit
distance 34N_119O2 :34@N :119@O2 out 34N_119O2.out
distance 73OG_119O3 :73@OG :119@O3 out 73OG_119O3.out
distance 12OG_119O14 :12@OG :119@O14 out 12OG_119O14.out
distance 28OH_119O14 :28@OH :119@O14 out 28OH_119O14.out

Plot the result. Here is the sample. It will be a good way to compare the H-bond distance with the binding free energy from MM-GBSA.



Create a new directory 005.MMGBSA To do an analysis we need three runs for the complex, ligand and receptor. Now write an input File: gb.rescore.in Single Point GB energy Calculation

 ntf=1, ntb=0, ntc=2,
 igb=5, saltcon=0.0,
 gbsa=2, surften=1.0
 offset=0.09, extdiel=78.5,
 cut=99999.0, nsnb=99999,
 scnb=2.0, scee=1.2,
 imin=5, maxcyc=1, ncyc=0,
  • idecomp=0 -> Important, but is turned-off here. It is used for analysis.
  • igb=5 -> OBC Flavor of GB
  • gbsa=2 -> Generalized Born / Surface Area
    • 1 -> LCPA Surface Area Method
    • 2 -> Recursive Atom-Centered Method
  • surften=1 -> Calculate Solvation Free-Energy (non-polar contribution)
  • offset=0.09 -> Dielectric Scaling for GB
  • extdiel=1.0 -> Dielectric Constant for Solvent Exterior (Default 78.5)
  • nsnb=99999 -> Non-Bonded List Update Frequency (See igb=0, nbflag=0) (Default=25)
  • scnb=2.0 -> 1-4 van der Waals Division (default=2.0)

Write the Following Job Script: run.sander.rescore.csh

#PBS -l nodes=1:ppn=2
#PBS -l walltime=24:00:00
#PBS -o zzz.mmgbsa.1.out
#PBS -e zzz.mmgbsa.1.err

set workdir = "${HOME}/AMBER_Tutorial/005.MMGBSA"
cd ${workdir} 

sander -O \
-i gb.rescore.in \
-o gb.rescore.out.com \
-p ../002.TLEAP/1df8.com.gas.leap.parm \
-c ../002.TLEAP/1df8.com.gas.leap.crd \
-y ../004.PTRAJ/1df8.com.trj.stripfit \
-r restrt.com \
-ref ../002.TLEAP/1df8.com.gas.leap.crd \
-x mdcrd.com \
-inf mdinfo.com \

sander -O \
-i gb.rescore.in \
-o gb.rescore.out.lig \
-p ../002.TLEAP/1df8.lig.gas.leap.parm \
-c ../002.TLEAP/1df8.lig.gas.leap.crd \
-y ../004.PTRAJ/1df8.lig.trj.stripfit \
-r restrt.lig \
-ref ../002.TLEAP/1df8.lig.gas.leap.crd \
-x mdcrd.lig \
-inf mdinfo.lig

sander -O \
-i gb.rescore.in \
-o gb.rescore.out.rec \
-p ../002.TLEAP/1df8.rec.gas.leap.parm \
-c ../002.TLEAP/1df8.rec.gas.leap.crd \
-y ../004.PTRAJ/1df8.rec.trj.stripfit \
-r restrt.rec \
-ref ../002.TLEAP/1df8.rec.gas.leap.crd \
-x mdcrd.rec \
-inf mdinfo.rec


Change "run.sander.rescore.csh" into an executable

:~> chmod +x run.sander.rescore.csh

Submit the job -> run.sander.rescore.csh

~> qsub run.sander.rescore.csh

Monitor your job

~> qstat -u YourUserName

Data extraction and calculation

When MD finised, you will find "gb.rescore.out.com", "gb.rescore.out.lig", "gb.rescore.out.rec" these three outputs. Use the following script to extract data of MMGBSA.

#! /bin/bash
# by Haoquan
echo com lig rec > namelist

LIST=`cat namelist`

for i in $LIST ; do

grep VDWAALS gb.rescore.out.$i | awk '{print $3}' > $i.vdw
grep VDWAALS gb.rescore.out.$i | awk '{print $9}' > $i.polar
grep VDWAALS gb.rescore.out.$i | awk '{print $6}' > $i.coul
grep ESURF   gb.rescore.out.$i | awk '{print $3 * 0.00542 + 0.92}' > $i.surf

paste -d " " $i.vdw $i.polar $i.surf $i.coul | awk '{print $1 + $2 + $3 + $4}' > data.$i

rm $i.*


paste -d " " data.com data.lig data.rec | awk '{print $1 - $2 - $3}' > data.all 

for ((j=1; j<=`wc -l data.all | awk '{print $1}'`; j+=1)) do
echo $j , >> time

paste -d " " time data.all > MMGBSA_vs_time

rm namelist time data.*

Run this script (it takes about 5 seconds) Now you have the final data sheet: MMGBSA_vs_time. Copy them to excel or Origin and separate two columns by comma. Result may look like this sheetand this graph.