Can You Capture Colors on Consecutive Nights with a Telescope?

  • Context: Stargazing 
  • Thread starter Thread starter russ_watters
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Discussion Overview

The discussion revolves around the challenges and techniques of capturing astronomical images over consecutive nights using a telescope, specifically focusing on color imaging and luminance data. Participants share their experiences with different imaging setups, filters, and software used for stacking images.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant mentions using Registax for aligning and stacking images but notes its limitations with field rotation, suggesting that data should ideally be collected in one night.
  • Another participant shares their experience of capturing color data over consecutive nights and emphasizes the importance of keeping the camera attached to avoid rotation issues.
  • There is a discussion about the use of hydrogen alpha filters for luminance imaging, with one participant explaining their method of replacing poor luminance data after a two-month gap.
  • A question is raised about the potential benefits of using an IR bandpass filter for luminance shots, suggesting it may reduce issues related to seeing conditions.
  • One participant clarifies that they use a UV/IR filter to make their images parafocal, indicating a specific setup involving stacked filters.
  • Another participant discusses the implications of using IR filters, noting that while they can be beneficial for certain types of imaging, they may cause issues like star bloating in nebula images.

Areas of Agreement / Disagreement

Participants express differing opinions on the use of IR filters and their effects on imaging quality, indicating a lack of consensus on the best approach for capturing luminance data. The discussion remains unresolved regarding the optimal filter choices for different astronomical targets.

Contextual Notes

Participants mention various limitations related to their imaging setups, including issues with tracking, exposure times, and the effects of atmospheric conditions on image quality. There are also references to specific software and techniques that may not be universally applicable.

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Jezz, sorry, been so long since I ues my scope I haven't looked in this thread! There is software out there that aligns and stacks images. I use Registax. It doesn't deal well with field rotation, so it is best to do all your data from each channel in one night.

I've done colors on consecutive nights, and combining them into an RGB image works best if the camera remains attached to the scope during the few nights of imaging so there aren't any rotation issues.

For luminance, I just went two months between capturing the color data and replacing some poor luminance data with better luminance data using a hydrogen alpha filter. So nothing about the camera setup was the same - not even the magnification. But it was relatively easy to rotate and stretch the luminance image in Photoshop.

Here's the full saga:
On 6/20 I shot:
14 exposures at 30 seconds for red (7 minutes)
27 exposures at 45 seconds for blue (20 minutes)
26 exposures at 45 seconds for green (20 minutes)

The red channel is more sensitive than the other two, so I use less exposure, though the number of exposures really should be equal. Also, tracking wasn't very good that night, so I had to discard a lot of frames. Still, the overall exposure time was a little on the low side. My first attached image is the resulting RGB.

I then shot:
34 exposures at 2 min for luminance (1:08 total) the same night.

Due to my bad tracking, the stars came out egg-shaped. So the second attached image is the combined lrgb. Not terrible, but the egg-shaped stars are a dealbraker to me. Plus the exposure time seemed a little low - the detail wasn't great.

Then I had two solid months of clouds, during whcih the telescope was set up in my living room. Last night was the first good night of sky(and perfect tracking) in months, and I shot:

26 exposures at 4 min each with a hydrogen alpha filter (1:44 total).

The third image is the result of combining that luminance image with the earlier color data. It's just under 2.5 hours of data altogether. I really could have used longer subs for the color, but it is good enough I'm not going to redo it for a long time. This was the first target I ever imaged (last year) and I've spent way too much time on it trying to get a good one as I climbed the learning curve. My first attempt is here, earlier in the thread (11 months ago): https://www.physicsforums.com/showpost.php?p=1097341&postcount=148
 

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russ_watters said:
...For luminance, I just went two months between capturing the color data and replacing some poor luminance data with better luminance data using a hydrogen alpha filter. So nothing about the camera setup was the same - not even the magnification. But it was relatively easy to rotate and stretch the luminance image in Photoshop...

...I shot:
26 exposures at 4 min each with a hydrogen alpha filter (1:44 total)...

Russ,

Have you ever tried to shoot the luminance shots using an IR bandpass filter instead of the H alpha? I've heard that the IR image is less subject to seeing problems.
 
All of my images are shot with a uv/ir filter, including the Ha. I do that to make them parafocal, since the Meade color filters pass uv and ir. So I have stacked filters (one on the nosepiece of the camera, and one in a rack).
 
Oh, you mean one that just let's through IR, not one that blocks it - right. Misread.

It is my understanding that you want to block the IR for images of nebulas because stars shine so bright in IR that they'll drown out the nebula. The stars get bloated. That seems to fit with my experience.

For galaxies, you need all the light you can get, and imaging in IR only doesn't give much signal. The second link you provided shows that.

Actually, about the only time you even want to include the IR at all is if you are imaging only stars or planets (though even for planets, the resolution is lower in IR because of the wavelength).
 

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