Hello,
I have some old data of NGC6888, which includes images for red, green, blue, OIII and Ha channels. The data is properly bias and dark calibrated, but the flat calibration is not perfect. It appears that dust motes calibrated out mostly (enough so that they are fainter than any of the data in which I'm interested), but the integrated master frames still show a significant radial gradient. The data was collected in under very dark skies and there is virtually no gradient other than what appears to be over-corrected vignetting.
Using DBE, I am able to get a good background model from the blue channel. For other channels though, particularly Ha, there is no part of the frame that is free of interesting signal.
Since the nature of the illumination error seems to be mostly the same in all channels, I would like to be able to use the background extracted from the blue channel to correct the illumination in all of the other channels.
Is there a way to do this with DBE, or will I need to build a PixelMath expression and do it manually?
Any suggestions?
Thanks,
-Wade
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