Difference between revisions of "Team:Aix-Marseille/SN"

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The with a RFP plasmid as a control we show there's no decrease.
 
The with a RFP plasmid as a control we show there's no decrease.
  
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Revision as of 23:30, 1 November 2017

SuperNova activity


We wanted to test the activity of [http://parts.igem.org/Part:BBa_K1491018 Supernova] on the colonies, so we made a protocol where we illuminated petri dish with a 16,5 Candela 595nm Diode (lumex ssl-lx5093syc/g) for 2 hours.

With the following protocol :

  • Transform 100µL TG1 with Eprc - SN (psb1C3 plasmid, 5µL)
  • To get an adequate number of colonies :
  • Into 2mL LB add 2µL of 2 DO TG1
  • Pipet up and down
  • From the first dilution, take 8µL and dilute it into 1mL LB
  • Spin at 5000rpm for 10min
  • Remove 850µL supernatant
  • Resuspend pellet (even if you can't see it)
  • Spread remaining 150µL on petri dish
  • Immediatly put on 590nm light / put control in dark
  • After two hours, incubate overnight
  • Count colonies


The with a RFP plasmid as a control we show there's no decrease.

Exposed Not exposed
Supernova 1496 3672
RFP 3545 3638


With this experiment, we can conclude that supernova allows us to divide the number of colonies by 2,45.