After acquiring my monochrome ATK16 IC camera I had to learn how to make colour images with this camera, which is amazing enough in its own right: making colour images with a b/w camera!
This technique is called 'LRGB' and is based on using colour filters during imaging and special post processing techniques.
During my learning curve I have made some notes, so that I would not forget what I learned.
No, this is NOT a full fledged LRGB Tutorial, but only describes the main scenario flavoured with some hints and tips.
IMPORTANT: for my DSO Tutorial - with many imaging and processing tips - click .... HERE !!!!
L R G B
L R G B
For fine tuning the exposure times between the filters you need to CALIBRATE the filters.
Jim Thommes said about this issue:
"If you image a G2V star with equal times for R,G,B (probably intentionally defocused) you should get a balanced colour. (i.e. at half max, each colour should have a weight of 128). If there is no balance, you can use Curves in Photoshop (at input level 128) to balance these colours for your test exposure. Record the output setting and now you have a scale factor for calibrated colours for use in Photoshop . Now you can relax an take all your filter exposures at the same time and calibrate them later in Photoshop."
Photoshop Tutorial by Jerry Lodriguss
More about calibration and also a list of G2V stars (sorted in RA).
There is a LOT more to say about this, but Rob Kantelberg has a nice Tutorial about this subject on his website [Tutorials => LRGB imaging. He even supplies an exposure calculator !].
L R G B
Meanwhile I have accumulated some experience myself in imaging with my ATK16IC camera, so here it is:
Note: because I am already familiar with K3CCDTools I decided to use K3CCDTools as my imaging software

|
Live Histogram At the top you see the L and H values: these are the actually measured values of the just captured image. At the bottom are also L and H values: these were manually selected by using the slider, so that I could get some preview. When you select "AUTO" the top and bottom values will be (almost) identical, depending on atmospheric conditions. |
L R G B
1. Align - Stack - FITS Liberator.
I align and stack the LRGB individual AVIs with K3CCDTools [see "Selecting, Aligning and Stacking" in my DSO Tutorial] and save as individual FIT files: 16 bit signed.
The next step is to bring out the details with the Photoshop Plugin FITS Liberator.
I highly recommend this plugin, which is freely downloadable; I also recommend the FITS Liberator Tutorial by Noel Carboni.
I save each file as a TIFF file with the suffix "fitslib", so that later I know that this is the result of the FITS Liberator processing.
2. Combining the R G B channels.
Don Waid has a tutorial about this Channel topic.
In short: in Photoshop open a new canvas, RGB, 16 bits and of the proper size.
Select: Window - Channels and you see a panel with the combined RGB and also the R G B separately.
Paste your Green image into the Green channel, Red into Red and Blue into Blue.
I usually have to manually align the channels, which is very easy with the arrow keys on your keyboard.
Hint: activate/deactivate the channel you are working on for blink comparison and fine adjustment.
Currently this is rapidly becoming my favourite scenario.
I save the result as: RGB-aligned.psd
When you are happy with the RGB result just add the Luminosity layer in the same fashion.
Hint: use about 50% Opacity of the Luminosity layer for proper positioning, then put Opacity at 100% and set the Blend mode to Luminosity.
I save this result as: LRGB-aligned.psd
3. How to avoid the "peach" or "salmon" hues of emission nebulae.
When you have mastered the above you will want to avoid "peach" or "salmon" hues of emission nebulae for which Robert Gendler has a very nice tutorial to include the h-alpha layer directly into the RGB colour data.
For my own convenience I have made the following extract telling me what to do:
4. Combining 2 Different Exposures.
Jerry Lodriguss has a fine tutorial about Combining 2 Different Exposures which is especially useful for objects with large differences in brightness, such as M42.
1. Removing halos by using the Inverse Selection method.
My good friend Adrian Jones had imaged the Double Cluster but wound up with blue halos around the brighter stars.
I gave it a try and here is my Photoshop scenario (of course I use Adrian's image with his full consent).
I slightly downsized Adrian's image so that it fits better on my screen ...
|
The image as captured and post processed by Adrian Jones. The blue halos are prominently present. |
Step 1: Select - Color Range - click on saturated star - slider at 192
Step 2: Select - Modify - 2 pixels (I used 2 pixels because of the size of the halos)
Step 3: Select - Inverse
Step 4: Hue/saturation(Ctrl-U) to de-saturate and darken the blue [one might do the same with red, which I did not do yet, but I invite you try do this yourself]
Step 5: Next I sharpened a bit [Filter|Unsharp Mask], which increased the brilliance.
Step 6: The Result
|
The blue halos have disappeared. |
|
This blink comparison shows the before and after ... |
Adrian Jones commented as follows:
Excellent, Jan!
Your method avoids the matching-back difficulty altogether by working on
the halos AND whole sky background together - very clever.
And it even flattens out slight colour unevenness in the sky background at the same time
- an extra bonus!
I'm really impressed by the results and will certainly use this method in
future for star clusters.
2. Removing halos while leaving a galaxy untouched.
This tutorial is an extension to my "Removing halos by using the Inverse Selection method ".
My good friend Stephane Poirier had imaged NGC7331 but wound up with reddish halos around the brighter stars.
When using my "Removing halos by using the Inverse Selection method " also the Galaxy was affected, which we do not want of course.
The problem was how to add the Galaxy to the already existing selection.
Here is what I did ...
Step 1 and 2: as in : "Removing halos by using the Inverse Selection method ".
Now we have to add the Galaxy to the selection, which I did as follows:
Step 3: Activate the 'Magic Wand' function
Step 4: with the cursor in the image: do a right mouse click: you get a pop-up menu
Step 5: Select 'add to selection' and hold the SHIFT-key down (and KEEP it down !!!)
Step 6: Activate and use the Lasso tool - I used a feather of 20 pixels - (now also press the left mouse key) and encircle the galaxy
Step 7: Now you can release the SHIFT-key: the galaxy has been added to the selection!
Step 8 and 9: similar to Steps 3 - 5 in : "Removing halos by using the Inverse Selection method ", but this time I concentrated on the Red colour.
The Result: Here you see the 'before' and 'after' of this scenario (just move your mouse in and out t see the difference):
|
3. Enhancing nebulosity by using the Inverse Selection method.
I use a similar technique as in the previous paragraph, but with a twist :o)
4. Hi Pass Masking: bring out dust lanes.
For your (and my own) convenience: here is a quick scenario of Don Waid's Hi Pass Masking Tutorial
I followed this Hi Pass Masking method, with the following result (just move your mouse in and out to see the difference):
|
5. Sylvain Weiller's solution to deal with light pollution.
Sylvain lives in Paris and here is his PDARK Photoshop solution against light pollution.
6. How to remove a Gradient with IRIS.
Here is the IRIS Tutorial of which I followed the "Gradient removal on very wide field images" (mouseover shows it all):

7. Get Vibrant colours without increasing contrast.
Here is a link to a tutorial how to Get Vibrant colours without increasing contrast by using Lab colours.
Here you see the 'before' and 'after' of this 'Get Vibrant colours' scenario (just move your mouse in and out te see the difference):
|
8. From elongated to round stars.
In spite of your best tracking and/or guiding you sometimes wind up with egg-shaped stars, alas ...
Here is my scenario to turn your eggs into nice round stars (but apply with care !!):
|
And here is the final image:
9. Bring out the colours of bright stars.
And Don Waid gives live demonstrations and explanations of what he does in Photoshop.
Here is in short steps what Don recommends to do to bring out the colours of bright stars:
L R G B
|
M67 - Open Cluster. First Light for my ATK16IC and also my first LRGB image. March 25, 2007 19:31 - 20:32 UT. I selected M67 because it contains a G2V star: nice to calibrate my filters. Imaging: William Optics Zenithstar 80 ED II APO, f/6.8 [focal length 545 mm] with 10 cm extender, Astronomik LRGB filters; ATK16IC b/w camera, K3CCDTools. Exposures: Luminosity 5x210 seconds; RGB 5x100 seconds; all unguided. |
|
M67 - Open Cluster. March 26, 2007 19:46 - 20:16 UT. My second LRGB image; once more I selected M67 because it contains a G2V star: nice to calibrate my filters. Imaging: William Optics Zenithstar 80 ED II APO, f/6.8 [focal length 545 mm] with 10 cm extender, Astronomik LRGB filters; ATK16IC b/w camera, K3CCDTools. Exposures: Luminosity 18x30 seconds; RGB 10x30 seconds; autoguided. |
|
M67 - Open Cluster. March 25, 2007 19:34 - 19:59 and March 26, 2007 19:46 - 20:16 UT. My first LLRGB image: I combined the 210 seconds luminosity layer of March 25, 2007 with the 30 seconds LRGB image of March 26, 2007. I determined the rotation between the images with Astrowave and then applied the exact rotation in Photoshop and layered. Imaging: William Optics Zenithstar 80 ED II APO, f/6.8 [focal length 545 mm] with 10 cm extender, Astronomik LRGB filters; ATK16IC b/w camera, K3CCDTools. Exposures: Luminosity 5x210 seconds plus18x30 seconds; RGB 10x30 seconds. |
The following QCUIAG friends helped me getting started in LRGB:
Dave Nash (Dave's LRGB page is here)
Jim Thommes
Peter Lloyd
Rob Kantelberg