![](Image\IMG_0994.jpg)
![](https://static.igem.org/mediawiki/2019/b/bb/T--NAWI_Graz--robettaaimodel1.png)
![](https://static.igem.org/mediawiki/2019/7/78/T--NAWI_Graz--aiplot1.png)
Figure 1: Robetta ab initio calculation model1 of g17 with estimated angstroms error per residue. In the structure T211 and W256 are highlighted.
![](https://static.igem.org/mediawiki/2019/2/2c/T--NAWI_Graz--robettaaimodel2.png)
![](https://static.igem.org/mediawiki/2019/8/82/T--NAWI_Graz--aiplot2.png)
Figure 2: Robetta ab initio calculation model2 of g17 with estimated angstroms error per residue. In the structure T211 and W256 are highlighted.
![](https://static.igem.org/mediawiki/2019/c/cb/T--NAWI_Graz--robettaaimodel3.png)
![](https://static.igem.org/mediawiki/2019/3/3f/T--NAWI_Graz--aiplot3.png)
Figure 3: Robetta ab initio calculation model3 of g17 with estimated angstroms error per residue. In the structure T211 and W256 are highlighted.
![](https://static.igem.org/mediawiki/2019/d/d1/T--NAWI_Graz--robettaaimodel4.png)
![](https://static.igem.org/mediawiki/2019/e/e5/T--NAWI_Graz--aiplot4.png)
Figure 4: Robetta ab initio calculation model4 of g17 with estimated angstroms error per residue. In the structure T211 and W256 are highlighted.
![](https://static.igem.org/mediawiki/2019/6/6b/T--NAWI_Graz--robettaaimodel5.png)
![](https://static.igem.org/mediawiki/2019/3/3f/T--NAWI_Graz--aiplot5.png)
Figure 5: Robetta ab initio calculation model5 of g17 with estimated angstroms error per residue. In the structure T211 and W256 are highlighted.