Jump to content

NLCbanner2024.jpg.2478be509670e60c2d6efd04834b8b47.jpg

Why does my background look like this?


Recommended Posts

Hi all. I tried photographing the Bode's and Cigar galaxy last night under Bortle 9 skies, but my final stacked image had a really mottled background after gradient subtraction in siril. Even before gradient removal, my background still looked quite horrible. Can anybody offer a possible explanation for this? My 30-second subs were quite washed out in the beginning but got a little bit better as the target rose above the skyglow of my area. Any help would be appreciated. Thanks!

Screenshot 2021-02-22 at 1.21.09 PM.png

Link to comment
Share on other sites

  • 2 weeks later...

The stripes are walking noise most likely caused by not dithering as Miguel said.

The inconsistent (not flat) background can have a number of causes, especially if your setup has light leaks or reflections which makes background subtraction much more difficult.

I don't know anything about siril,  but if I got a background like this I would he looking for samples placed too close to stars in the dark areas which are then fooling the background modelling prior to subtraction.

APP can do a decent job but the nuclear option is something called a synthetic flat in PI. This will flatten the background although I don't think it will help with the walking noise:

http://trappedphotons.com/blog/?p=756

Link to comment
Share on other sites

Create an account or sign in to comment

You need to be a member in order to leave a comment

Create an account

Sign up for a new account in our community. It's easy!

Register a new account

Sign in

Already have an account? Sign in here.

Sign In Now
  • Recently Browsing   0 members

    • No registered users viewing this page.
×
×
  • Create New...

Important Information

We have placed cookies on your device to help make this website better. You can adjust your cookie settings, otherwise we'll assume you're okay to continue. By using this site, you agree to our Terms of Use.