Interesting. This has great potential, though to understand whether the results can be used for scientific analysis and for example contribute to the VSS database, I hope they publish information about how it is doing the photometry. Things like does it check for saturation and keep the counts within the linear response region of the chip, is it using the green channel to approximate V, what comparison star magnitudes are being used and how are the comparison stars chosen. Without this it is still a fantastic innovation and could get more people into variable star observing.
Andy (BAA VSS Database Secretary)