For our user-friendly kit we required a circuit which displayed a simple on/off output once a certain level of DCM had been reached. The biochemists attached super-folder green fluorescent protein (sfGFP) to the promoter region of dcmA, such that when DCM is present, the bacteria fluoresce.
![](https://static.igem.org/mediawiki/2014/3/33/Oxford_emission_graph.jpg)
After initially assuming that GFP fluoresces on its own, the biochemists informed me that it needed to be excited by a specific wavelength of light. For our project we chose to use sfGFP as it folds more robustly than regular GFP. sfGFP has an absorption peak at 485nm and an emission peak at 520nm. Whilst there was plenty of data for GFP, sfGFP absorption and emission spectra data could not be found. As such, we have used the spectra for eGFP which we believe to be very similar to that of sfGFP. As can be seen in the 'GFP Emission/Absorption' diagram, the absorption (blue) and emission (green) spectra cover quite a range of wavelengths with considerable overlap around the 500nm region. This overlap requires careful consideration in the design of the overall bio-detection kit as the excitation and emission light will mix and become indistinguishable to unfiltered sensors.
![](https://static.igem.org/mediawiki/2014/d/d3/Oxford_rainbow_graph.jpg)
The configuration in our end product will follow that shown in the 'Component set up' diagram. We will use blue LEDs to excite our sfGFP, which are ideal because they emit light in the range 450-500nm and are very cheap. Photodiodes are highly sensitive to the direction of the incoming light, so we will manipulate the circuit such that the LEDs lie at right angles to the photodiodes to reduce the amount of incident blue light.
The mix of the blue excitation from the LED and the green emission light from the sfGFP will then be passed through a filter which has the absorption spectra shown in the 'Filter absorption spectra' diagram. This filter will absorb a large amount of the blue light and little of the green light, so that a larger portion of the incident light on the photodiode is the signal we want to measure. We can calibrate our photodiode to ignore the small amounts of blue light transmitted through the filter, by taking light measurements in the absence of sfGFP.
![](https://static.igem.org/mediawiki/2014/6/6a/Oxford_light_circuit.png)
To simplify the electrical analysis, I will talk about the voltage levels at varying points throughout the circuit with two different light levels, light and dark.
A. When light is incident on the photodiode, a small voltage is created across its terminals. This voltage is immediately amplified by 10 to get a larger voltage at node A. (Using the BPW21 photodiode on the fifth floor of the Thom building, Vlight=4V and Vdark=-6V.) The voltage produced at A is now a sizeable amount but it is offset from 0V, which will make further analysis harder.
B. Using a voltage divider resistor network, we created a fixed voltage point equal to the dark voltage offset at A. We put an OP-AMP setup as a voltage follower between this and the next part of the circuit, to isolate the network and ensure that the voltage level created wasn’t affected by any circuitry downstream. This fixed voltage (-6V) can be measured at the node labelled OFFSET. We inputted the voltages A and OFFSET into a unity gain comparator. Which created a voltage at B which follows the equation B=OFFSET - A. By having the OFFSET equal to Vdark, it will cause the voltage for one of the light levels to be 0V. (At node B, Vlight=-10V and Vdark=0.)
C. If necessary we can amplify the voltage at B again using the non-inverting amplifier which has a gain which follow the equation: Gain=1+R10/R9. With the resistor values seen in the circuit diagram, the gain=10. Although the maximum voltage we can produce is limited by the OP-AMP’s inability to provide voltages larger than the power rails which supply it (+/-15V). So if we are using the BPW21 no further amplification is required, so I removed R9 so that the gain was reduced down to Gain=1. (At node C, Vight=-10V and Vdark=0V).
D. For the final stage, we created another fixed voltage point which will control the threshold light level (-5V). Since the last OP-AMP has no feedback, the gain is effectively infinite and the output will saturate to the power rails. When the voltage at C is larger than -5V (Vdark=0), the output of the OP-AMP will saturate positively causing the voltage at node D= +15V. This will cause the green LED to illuminate, indicating that it is safe to pour down the sink as there is no light being produced, as there is no SFGFP present because there is no DCM left. When the voltage at C is lower than -5V (Vlight=-10), the output of the OP-AMP will saturate negatively causing the voltage at node D=-15V. This will cause the red LED to illuminate, indicating that it is not safe to pour down the sink as light is being produced, since there is GFP present because some DCM is still present.
As desired, we have a simple binary output which shows the user when the liquid is safe to pour down the sink.