Difference between revisions of "Team:Austin LASA/Model"

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       h(g.Image, {src: 'https://static.igem.org/mediawiki/2018/6/6b/T--Austin_LASA--Tp_8_6.svg', position: 'center'}),   
 
       h(g.Image, {src: 'https://static.igem.org/mediawiki/2018/6/6b/T--Austin_LASA--Tp_8_6.svg', position: 'center'}),   
 
       h(g.Image, {src: 'https://static.igem.org/mediawiki/2018/0/06/T--Austin_LASA--Tp_8_8.svg', position: 'center'})     
 
       h(g.Image, {src: 'https://static.igem.org/mediawiki/2018/0/06/T--Austin_LASA--Tp_8_8.svg', position: 'center'})     
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      h('p', null, 'The data for primer sets 14, 573, and 12 were clearly linear as expected, and the linear regression for primer set 11 is still close enough to give a meaningful value for slope. We use the slopes of these regressions as a measure of the effectiveness of the primer set, with a higher magnitude corresponding to a greater primer effectiveness. Primer set 14 had a significantly higher slope magnitude than the other sets, so we can conclude that it will be the most effective primer for amplifying our HIV sample with LAMP.')
 
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Revision as of 08:43, 17 October 2018