Hi everyone,
Every since I have started mono imaging, I have been plagued with prominent and large halos around (very) bright stars. See for yourselves on these LRGB stacks of LEO I, next to Regulus: Reflection.jpg
It appears to be especially noticeable in the green channel. Please note I cannot rule out dew and/or high clouds for the less sharp halos.
The images were captured using a 200 mm f4 newtonian with a Paracorr II, bringing the focal length to around 920 mm. Astronomik L2 and Deep Sky RGB were used in front of a ASI2600MM camera.
In order to try and diagnose the source of the reflections, I came acress this archived article from Astrodon, which describes a method to locate the reflection in the imaging train: https://web.archive.org/web/20140729003031/http://www.astrodon.com/articles_faq/articles_faq/press_release:391,355,49
In the green channel, I measured the halo to be approximately 1340 pixels wide, which ultimately leads me to a reflection distance of ~23 mm from the sensor. As per the article, this number has to be divided by 2 to get the physical distance, so ~11.5 mm. Accounting for the measurement errors, we get dangerously close from the distance between the front of the camera (without the tilt plate, which I removed) and the sensor itself.
I’m not really sure my method is sound, but would I be right to suspect the AR window of the camera, or its interaction with the filters? And, most importantly, is there anything I can do to resolve this issue, without resorting to buying new filters?
I would be very interested in hearing your opinions and any advice you would have.