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+ | <p>Our Modelling workflow could be summed up as :</p> | ||
+ | </div> | ||
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+ | <p>Two hackathons to screen the most promising cores and AMPs based on rationnal criteria</p> | ||
+ | </div> | ||
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+ | <p>Homology modeling of the 210 constructs with Modeller on Pymol</p> | ||
+ | </div> | ||
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+ | <div class="textbody"> | ||
+ | <p>Molecular Dynamic simulations to test the stability of the predicted structures using Yasara and Inserm Cluster</p> | ||
+ | </div> | ||
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+ | <p>Followed by cores and AMPs selection, we were interested in determing the model of the fusion. This led us to the modeling expert, Antoine Tally, who guided us to standardise a protocol for our analysis. Aim: To construct an atomic-resolution model of Star-core monomer via comparative homology modelling</p> | ||
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+ | <p>Making fusion protein of 2 known PDB files using CHIMERA</p> | ||
+ | </div> | ||
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+ | <h4>Monomer construct on Chimera using Modeller graphic interface</h4> | ||
+ | </div> | ||
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+ | <h4>construct optimization on Chimera</h4> | ||
+ | </div> | ||
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+ | <h4>Superpozition on Pymol thanks to handmade script called <a href="http://Superpoz.py" target="_blank">Superpoz.py</a><br></h4> | ||
+ | </div> | ||
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− | + | <p>OBJECTIVE: </p> | |
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− | < | + | <p>-Study behaviour of fusion molecule in vicinity of cell.</p> |
− | < | + | </div> |
− | </ | + | <div class="textbody"> |
+ | <p>-Assess the stability of Star cores in terms of protein folding, structural characteristics and energy.</p> | ||
+ | </div> | ||
+ | <div class="textbody"> | ||
+ | <p>-Define constraints and parameters for simulations.</p> | ||
+ | </div> | ||
+ | <div class="textbody"> | ||
+ | <p>-Use Yasara to analyze MDS data.</p> | ||
+ | </div> | ||
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<h2>CONCLUSION</h2> | <h2>CONCLUSION</h2> | ||
</div> | </div> | ||
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+ | <p>In this project, we combinatorially fused a set of known AMPs to structurally diverse, self-assembling protein cores to produce star-shaped complexes.</p><p>We selected 14 cores that already exist and 15 AMPs, hence over 200 fusions were designed and expressed in a cell-free system, then screened for activity, biocompatibility, and membrane selectivity.</p><p>To study the behaviour of in-vitro synthesised molecules we designed the fusion molecules for all constructs using Chimera, Modeller and Pymol. We visualized the assembly and fusion monomer (core + AMP) and studied their behavioural attributes, changes in folding of alpha helix and beta sheath using Yasara as it mimics atom behaviour in real life. Using visualization and MDS studies we confirm that proteins folds well and on an average maintain constant RMSF (Root Mean Square Fluctuations) with all amino acid residues, also expressed well in cell free system.</p> | ||
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+ | <h2>METHODS</h2> | ||
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+ | <h4>These protocols were defined under certain parameters:</h4> | ||
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<ul> | <ul> | ||
<li> | <li> | ||
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<p>However we verified this hypothesis with our stability MD assay developped with Marc Baaden.</p> | <p>However we verified this hypothesis with our stability MD assay developped with Marc Baaden.</p> | ||
</li> | </li> | ||
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− | <p>Homology modelling is comparative modelling of proteins. It is a comparative protein modelling method designed to find the most probable structure for a sequence given its alignment with related structures. The three-dimensional (3D) model is obtained by optimally satisfying spatial restraints derived from the alignment and expressed as probability density functions (pdfs) for the features restrained. For example, the probabilities for main-chain conformations of a modelled residue may be restrained by its residue type, main-chain conformation of an equivalent residue in a related protein, and the local similarity between the two sequences. Several such pdfs are obtained from the correlations between structural features in 17 families of homologous proteins which have been aligned on the basis of their 3D structures. The pdfs restrain C alpha-C alpha distances, main-chain N-O distances, main-chain and side-chain dihedral angles. A smoothing procedure is used in the derivation of these relationships to minimize the problem of a sparse database. The 3D model of a protein is obtained by optimization of the molecular pdf such that the model violates the input restraints as little as possible. The molecular pdf is derived as a combination of pdfs restraining individual spatial features of the whole molecule. The optimization procedure is a variable target function method that applies the conjugate gradients algorithm | + | |
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+ | <div class='textbody h4'> | ||
+ | <h4>Homology Modelling</h4> | ||
+ | </div> | ||
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+ | <div class='textbody'> | ||
+ | <p>What is homology modelling?</p> | ||
+ | </div> | ||
+ | |||
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+ | <p>Homology modelling is comparative modelling of proteins. It is a comparative protein modelling method designed to find the most probable structure for a sequence given its alignment with related structures. The three-dimensional (3D) model is obtained by optimally satisfying spatial restraints derived from the alignment and expressed as probability density functions (pdfs) for the features restrained. For example, the probabilities for main-chain conformations of a modelled residue may be restrained by its residue type, main-chain conformation of an equivalent residue in a related protein, and the local similarity between the two sequences. Several such pdfs are obtained from the correlations between structural features in 17 families of homologous proteins which have been aligned on the basis of their 3D structures. The pdfs restrain C alpha-C alpha distances, main-chain N-O distances, main-chain and side-chain dihedral angles. A smoothing procedure is used in the derivation of these relationships to minimize the problem of a sparse database. The 3D model of a protein is obtained by optimization of the molecular pdf such that the model violates the input restraints as little as possible. The molecular pdf is derived as a combination of pdfs restraining individual spatial features of the whole molecule. The optimization procedure is a variable target function method that applies the conjugate gradients algorithm to positions of all non-hydrogen atoms. The method is automated. We used modeller to predict all our models. The steps are: </p> | ||
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<table> | <table> | ||
<thead> | <thead> | ||
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</thead> | </thead> | ||
<tbody></tbody> | <tbody></tbody> | ||
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− | For this workflow we will use:</p><ul> | + | |
+ | |||
+ | |||
+ | <p>For this workflow we will use:</p><ul> | ||
<li>UCSF-CHIMERA : download link</li> | <li>UCSF-CHIMERA : download link</li> | ||
<li>MODELLER: online or installed</li> | <li>MODELLER: online or installed</li> | ||
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Figure : Simulation of fusion monomer ferritin + ovispirin (4XGS + 1HU5) | Figure : Simulation of fusion monomer ferritin + ovispirin (4XGS + 1HU5) | ||
</code></pre><h4 id="Parameters-">Parameters :</h4><ul> | </code></pre><h4 id="Parameters-">Parameters :</h4><ul> | ||
− | <li>pH at which the simulation should be run, by default physiological pH 7.4<br> | + | <li> -pH at which the simulation should be run, by default physiological pH 7.4<br> |
The ion concentration as a mass fraction, here we use 0.9% NaCl (physiological solution)ions=‘NaCl,0.9’</li> | The ion concentration as a mass fraction, here we use 0.9% NaCl (physiological solution)ions=‘NaCl,0.9’</li> | ||
− | <li>Simulation temperature, 298K</li> | + | <li> -Simulation temperature, 298K</li> |
− | <li>Water density = 0.997</li> | + | <li> -Water density = 0.997</li> |
− | <li>Duration of the simulation = 15ns</li> | + | <li> -Duration of the simulation = 15ns</li> |
− | <li>Extension of the cell on each side of the protein ‘10’ means that the cell will be 20 A larger than the protein.<br> | + | <li> -Extension of the cell on each side of the protein ‘10’ means that the cell will be 20 A larger than the protein.<br> |
Shape of the simulation cell: ‘Cube’.</li> | Shape of the simulation cell: ‘Cube’.</li> | ||
− | <li>Forcefield : ForceField AMBER14</li> | + | <li> -Forcefield : ForceField AMBER14</li> |
− | <li>Cell boundary : Boundary periodic<br> | + | <li> -Cell boundary : Boundary periodic<br> |
The simulation speed, ‘fast’ (maximize performance with 2*2.5 fs timestep and constraints)<br> | The simulation speed, ‘fast’ (maximize performance with 2*2.5 fs timestep and constraints)<br> | ||
The save interval for snapshots. Normally you don’t need more than 500-1000 snapshots of your simulation.<br> | The save interval for snapshots. Normally you don’t need more than 500-1000 snapshots of your simulation.<br> |
Latest revision as of 03:30, 18 October 2018
Modeling
INTRODUCTION
Our project is based on the consequences of conformational change of antimicrobial peptides. Results generated by the testing group showed that MIC is not a reliable criteria to understand the activity of our StarCores while it has been previously used for species. It was crucial to have some models to:
Determine which constructs would be interesting | ||
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Interpret our experiments results |
1. Obtain reference PDB structures representing the core and antimicrobial peptide protein monomers | 2. Use MODELLER via CHIMERA interface for homology modelling | 3. Choose the best fusion protein model that represents the Star core monomer |
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