Team:UNIPV-Pavia/Material Methods/Measurements/Tecan/test28settembre
From 2010.igem.org
m (→RESULTS) |
m (→RESULTS) |
||
Line 71: | Line 71: | ||
[[Image:UNIPV10 SScellM28settembre.png|thumb|500px |center|Mean of (dGFP/dt)/O.D.600 (under the hypothesis that GFP half-life in fusion contructs is similar to the original one - <partinfo>BBa_E0040</partinfo>)]] | [[Image:UNIPV10 SScellM28settembre.png|thumb|500px |center|Mean of (dGFP/dt)/O.D.600 (under the hypothesis that GFP half-life in fusion contructs is similar to the original one - <partinfo>BBa_E0040</partinfo>)]] | ||
- | All cell cultures showed a similar growth curve | + | All cell cultures showed a similar growth curve; doubling time was computed as described [[Team:UNIPV-Pavia/Parts/Characterization#Doubling_time_evaluation|here]] in order to have informations about the burden due to synthesis of such fusion proteins. It's possible to see that all doubling time are very similar except for induced cultures. In this case doubling time is much higher than positive control and not induced cultures; so it's possible to assert that in this case there's a kind of metabolic burden higher than in the others, maybe because of the inducible system. |
From GFP curve it's possible to appreciate that in induced I63, I64 and I65 GFP accumulation profile it's very similar and it's significantly different from that of negative control <partinfo>BBa_B0031</partinfo>. On the other hand not induced I63 and I64 show a profile very similar to the last one. This result that the green fluorescent protein assembled downstream of the genetic circuit is correctly folded. | From GFP curve it's possible to appreciate that in induced I63, I64 and I65 GFP accumulation profile it's very similar and it's significantly different from that of negative control <partinfo>BBa_B0031</partinfo>. On the other hand not induced I63 and I64 show a profile very similar to the last one. This result that the green fluorescent protein assembled downstream of the genetic circuit is correctly folded. |
Revision as of 19:21, 27 October 2010
|
||||||||||||||||||||||||||||||||
|
|
|