Difference between revisions of "Team:Arizona State/Description"

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<p>AHLs share the same basic structure, with a lactone ring, an N-acyl and ketone group. The defining R group lies in the acyl tail, which is the primary determinant in its transcription factor binding affinity. The graphic below demonstrates the categorization of the AHLs produced by the 10 studied systems</p>
 
<p>AHLs share the same basic structure, with a lactone ring, an N-acyl and ketone group. The defining R group lies in the acyl tail, which is the primary determinant in its transcription factor binding affinity. The graphic below demonstrates the categorization of the AHLs produced by the 10 studied systems</p>
 
<center><img src="https://static.igem.org/mediawiki/2016/4/4f/T--Arizona_State--ahlcategory.png" height=500px></center>
 
<center><img src="https://static.igem.org/mediawiki/2016/4/4f/T--Arizona_State--ahlcategory.png" height=500px></center>
<h2>F2620 Inductions</h2>
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<p>The ASU team would like this experiment to be considered for the Gold Medal Requirement of improving the characterization of a previously existing BioBrick part. All 10 systems were studied in an induction test. The part BBa_F2620 (designed by Barry Canton from MIT) was used to induce production in the Lux AHL system and test induction in any other AHL systems. By studying interactions between the 10 constructed Senders and F2620, we were able to analyze the systems for potential orthogonality. The resulting part collection allows direct comparison in AHL induction between multiple systems. The Part Numbers for these Senders are
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<a href="http://parts.igem.org/Part:BBa_K2033000">BBa_K2033000</a>,
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<a href="http://parts.igem.org/Part:BBa_K2033002">BBa_K2033002</a>,
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<a href="http://parts.igem.org/Part:BBa_K2033004">BBa_K2033004</a>,
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<a href="http://parts.igem.org/Part:BBa_K2033006">BBa_K2033006</a>,
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<a href="http://parts.igem.org/Part:BBa_K2033008">BBa_K2033008</a>, which correspond to the Aub, Bja, Bra, Cer, and Sin systems.  We believe that this Part Collection is a valuable addition to the registry, because while small in size, it contributes 5 Senders to the registry which contains around 6 Senders. In addition, this will add information about these new systems to a well-characterized and widely-used part in F2620. Not only will this determine interactions between systems, but also, provide characterization information for any future quorum sensing research involving those systems.</p>
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<p>We also created Senders for the Esa, Las, Lux, Rhl, and Rpa systems, which already exist in the registry. These correspond to the following parts:</p>
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<ul>
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<li>EsaI-<a href="http://parts.igem.org/Part:BBa_K1670004">BBa_K1670004</a></li>
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<li>LasI-<a href="http://parts.igem.org/Part:BBa_C0178">Bba_C0178</a></li>
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<li>LuxI-<a href="http://parts.igem.org/Part:BBa_C0161">BBa_C0161</a></li>
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<li>RhlI-<a href="http://parts.igem.org/Part:BBa_C0170">BBa_C0170</a></li>
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<li>RpaI-<a href="http://parts.igem.org/Part:BBa_K1421006">BBa_K1421006</a></li>
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<p>We added the induction data that we collected for these systems to their respective parts pages, which provides information on their compatibility with F2620.</p>
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</div>
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<div class = "container">
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Revision as of 01:39, 2 November 2017