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Philippe, is there an issue with your website?  None of the images you post seem to show up, including your Avatar.  :sad:

Craig
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Gallery / Re: M101 Pinwheel Galaxy
« Last post by lucchett on Today at 14:55 »
Congratulations, nice colors!

For Ha blending, the ha script works nicely in my opinion.
It works well on galaxies, but you need to work hard on the background areas.
The only control missing is a range mask option to avoid the blending in low SNR areas.
For that reason, ha image must be very deep> otherwise you need to fight against a red noisy background.

if you find a way to run the script selectively, please tell me!


best regards,
Andrea
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You are correct about using monochrome images. The first post explains this, and yes, the work flow is not optimal on this point. I do not expect that anyone will use the manual work flow and use the BP script instead. This is all explained in the first post. I imagine that admin will remove it in due course. I am not motivated to make the changes - you are most welcome. Which is where I will leave the discussion ;)

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The BP script converts all RAW files to "CFA no deBayer monochrome images", which is preferable for calibration and avoids wildly excessive pixel rejection. A shortcoming of the DSLR_RAW work flow is that it does not describe this process.
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General / NoiseEvaluation script - dark current reduction
« Last post by astropixel on Today at 12:28 »
Long time since posting, but I need a little help interpreting the output of the NoiseEvaluation script for two Grayscale DSLR dark frames. What is the data telling me about the dark frames in practical terms?

I'm guessing, that the second frame has approximately 25% the dark current of the first frame. If so, I think that verifies the 14C difference between the frames at 17 and 3C.

Many thanks

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IMG_9158_RGB_VNG
Calculating noise standard deviation...

* Channel #0
?K = 1.584e-04, N = 7763639 (36.72%), J = 4

IMG_9168_RGB_VNG
Calculating noise standard deviation...

* Channel #0
?K = 1.086e-04, N = 13163121 (62.25%), J = 4
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Quote
The cornermask is, a you mentioned, an offense against the PI philosophy.

It depends on how and why you apply it. If by "PI philosophy" you mean my philosophy, then here it is. If you:

- Analyze the data to find and outline the problem,

- Understand the problem and its causes (for example, an ampglow artifact or a light leakage issue in this case),

- Design a suitable solution to the problem (a local mask in this case),

- Evaluate the side effects and the risks of your solution (decreased SNR on the masked area in this case, and the risk of introducing a nonuniform illumination artifact),

- Make an informed decision as to whether the solution of the problem is worth the side effects and risks,

- Apply the solution strictly to solve the problem, preferably in a purely algorithmic way,

- Evaluate the result of the applied solution and its side effects,

then what you are doing is astrophotography: Turning data into information to communicate something from nature. However, if you do one or more of the following:

- Apply arbitrary manual retouching techniques without documentary criteria (example: create a layer mask, paint it with a brush by hand, then sharpen where you want because it looks nicer that way),

- Remove objects or image structures selectively, without documentary criteria (for example, removing all the stars in a wide-field image can be a nice way of revealing the true shape of a nebula, but removing a large blooming by cloning its adjacent pixels is like "inventing" that part of the image),

- Add artificial elements or artifacts "for aesthetic purposes" (example: artificial star spikes),

- Apply any process selectively without documentary criteria, i.e. without criteria based on a thorough analysis and understanding of the properties and nature of the data and of the objects represented (typically also for aesthetic reasons),

- Apply processes incorrectly, or without the necessary knowledge and common sense, (typically, trying to process an image beyond the reasonable limits imposed by the SNR of the data),

then what you are doing is, to a lesser or greater extent, painting. Downloading the image from the Internet to modify it, or painting it directly on a canvas, may be easier than acquiring it from the sky, and the results may be aesthetically better, too.

Astrophotography, as I understand it, is much more about the "how" and the "why" than about the results. When I look at an image, I need to be sure that I can trust what I am seeing. For this to happen, I need to know how the image has been processed and why. In essence, this is also the philosophy behind PixInsight, but everybody can use a tool as they want.
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Good points Gerald. Thanks for clarifying.
Geoff
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Hi Geoff!
The cornermask is, a you mentioned, an offense against the PI philosophy. I fully agree. And i dont do it myself.
But for those who still think they need to move to PS for this kind of postprocessing they have one reason
less to move the data into the painting Programm and loosing data because of conversion...

My intention is to show that there s no need at all to do the "final tweaking" or "any "tweaking" in PS.
The move to the correct treatment and clean philosophy of handling data
will come more easy if PS is more and more visible obsolete.

Aloha
Gerald
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Like Sander I tested some tweaking from your settings
For sure TGV is the best followed by ACDNR !

But, if I got some better results with a little noise as I like in astronomy images, I don't think the square double gradient image is similar to an astronomy deep sky image challenge.
 
For example, in LINEAR images, noise reduction is best now with TGV followed by ATWT (only the k-sigma noise thresholding option)
For NON-LINEAR, for sure TGV, then ACDNR

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Very intriguing Gerald.  It will take some time to absorb the content in these two videos. I have one question concerning the mask that isolates just one corner of the image.  This seems a little like a hand painted mask in Photoshop.  What are your thoughts on how this fits in with the overall PixInsight philosophy?
Keep up the good work.  I look forward to the next video.
Geoff
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Gallery / Re: M101 Pinwheel Galaxy
« Last post by jeffweiss9 on Today at 04:42 »
I took your advice and redid the HaLRGB combination with Ha added to Red only, not Luminosity. Doing something like Vicent Peris's technique of subtracting from the Ha a fraction of the red and then empirically using that Ha to enhance the red, I think I got a better result than the original.   Located at the same link:

http://www.astrophotogallery.org/member-galleries/p11384-m101-pinwheel-galaxy.html

but the original is also at:

http://www.flickr.com/photos/9906726@N08/8749860539/in/photostream/

Thanks for the tip.
-Jeff
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