Over the last few months, under different sky conditions (varying brightness), I've been grabbing occasional short (1hr) OSC data sets of a variable star that will vary by approx 7 magnitudes. I'm hoping to compare the flux data with known light curves with Aperture Photometry on the green channel, but would also like to present the data as a sequence of images where the sky background level & (fixed magnitude) star sizes remain consistent. How can I do this? I've been thinking that I may need to integrate each nights data separately, apply DBE & SPCC, and then split into RGB channels. Then apply Linear Fit to each channel, recombine, and then apply the same stretching regime to each night's image. I'm not sure if this will work - any idea on alternative workflows? Is there a way to match the PSF of stars between images, so that the fixed bright stars appear ot be the same size?
Any ideas much appreciated - I think the variable star should reach it's peak magnitude in about a months time, so I'm still in the data aquisition stage at the moment...
Thanks
Ivor
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