Hello,
Are there any planned followups to the Fabian Neyer Star Removal videos in Horizons?
The method described does a good job of removing stars that follow a normal brightness distribution. But it does not remove significant diffraction effects from very bright stars. You can see this in the M27 image in the existing videos, where there are a handful of residual halos and spikes from the very brightest stars.
My interest isn't necessarily in diffraction spikes specifically. In my case, I am using an ASI1600MM-cool camera with a Panasonic sensor. The cover glass on the sensor does not have an anti-reflection coating, and there is a very distracting reflection artifact around very bright stars. Since it's real signal from light hitting the sensor, just like diffraction spikes, I'm making an assumption that techniques to remove diffraction spikes would be a good place to start.
In some cases, where there the star is colored, the effect may show up in one channel, but not another. The current project that I'm looking at is an HaOIIIRGB image of the Bubble Nebula. The star in question is SAO 20562, which is quite blue. The artifacts show up clearly in the OIII data, but not in similarly stretched Ha data. It's also present in the RGB masters.
My intention for the data is to do a bicolor of the narrow band data and use RGB color for the stars. I like the stars in the Ha master, and would like to remove the stars from the OIII prior to doing the bicolor blending, and than take only hue data from the RGB and apply it to the stars.
If you have any suggestion on how to approach removing complicated stellar artifacts, I would be interested in hearing about it. I would also be happy to make the calibrated and integrated masters available, if you would like to take a look, or even use them for a tutorial.
Thanks,
-Wade
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