Jump to content

SkySurveyBanner.jpg.21855908fce40597655603b6c9af720d.jpg

First go at NB and RGB blending


The Admiral

Recommended Posts

Recently I imaged the Horsehead in wide-band and dual-band with a OSC camera (https://stargazerslounge.com/topic/405602-yet-another-horsehead-nebula/#comment-4341481). I use APP, and the blending was a new venture. This wasn't as straightforward as I'd hoped, as registering the channels was problematic on account of the RGB and Ha images being of rather different sizes (don't ask!), and APP objected using the standard parameters. Anyway, eventually got that sorted.

The image represents some 2.5h on Ha, and 3.3h of wide-band, after weeding out the bad ones.

ASKAR FRA400 and ASI533MC camera on AM5 mount. ASIAir Plus.

WO 50mm guidescope with ASI120MC

Wide-band: 100x2m subs; Ha: 50x3m subs, using Optolong L-eXtreme.

Here is the result, processed in APP and finished in Lightroom.

2040047_IC434-HaRGB_1-2-St-6normal.jpg.8c6609631179be10e3cebcae21fac525.jpg

 

Thanks for looking.

Ian

  • Like 10
Link to comment
Share on other sites

13 hours ago, SteveNickolls said:

Would you try a different balance of using more Ha another time too add more detail?

Thanks Steve.

I think I know what you mean. If I look at the Ha image I can see a fair bit of detail that doesn't seem to have come through into the blended image. I'm not sure that just adding more of the Ha component will improve that though, as it'll just make more of the image red. When I next get the opportunity I'll tinker some more.

Ian

  • Like 1
Link to comment
Share on other sites

33 minutes ago, ollypenrice said:

I wonder what colour your broadband-only Flame was?

It is shown on my original images, if you follow the link I gave. It is a light yellowy- pink. Mind you, the colour correction my be a little off I guess. The Ha image, which is also on the link, appears to show the Flame to be quite a strong Ha emitter, and so I expected the nebula to turn more red.

No, I don't know exactly know how the Combine RGB tool works exactly. Not as obvious as the PS clearly, but I'm trying to stick with what I have for the moment.

Ian

Edited by The Admiral
  • Like 1
Link to comment
Share on other sites

17 hours ago, The Admiral said:

It is shown on my original images, if you follow the link I gave. It is a light yellowy- pink. Mind you, the colour correction my be a little off I guess. The Ha image, which is also on the link, appears to show the Flame to be quite a strong Ha emitter, and so I expected the nebula to turn more red.

No, I don't know exactly know how the Combine RGB tool works exactly. Not as obvious as the PS clearly, but I'm trying to stick with what I have for the moment.

Ian

Yes, I see in the link that your original Flame is the classic colour. The addition of Ha doesn't normally change it by much, I don't think, either in PI or Ps.

Olly

Edit: I only focus on this because Ha blending is mentioned in the title. It's a good image.

Edited by ollypenrice
Stated
  • Thanks 1
Link to comment
Share on other sites

With the simplistic notion that luminance is detail rather than colour, I thought I'd try using some luminance data in the mix. Fiddling with the mix parameters of the channel mixer, a completely naive empirical approach on my part, I produced this. I think it's better in that the Flame is not reddened there is more of the dust apparent. Not sure that there is more detail visible in the Ha curtain, and Alnitak isn't so well resolved.

I think I have rung as much as I can out of this data.

IC434_HaRGB-HaRGB_1-St-9_2.jpg.2785a4ca8ba1627713b81a7c27dd5074.jpg

 

Thanks again for looking.

Ian

  • Like 2
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.