Image Processing Tutorial #3 This tutorial assumes you have a pre-stacked group of raw files. The example uses a stack of IC1848 images captured thus: There is moderate light pollution at my site (suburban Santa Barbara, CA). Shooting date: September, 2007. Astronomical image processing is a simple series of small steps. Stretch the histogram a little, apply noise reduction, repeat. This tutorial is aimed at producing images from underexposed raw files. Such files are common when shooting unguided exposures or as a mean to inhibit overexposure due light pollution. Both require short exposures. |
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Dialogue Settings
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The unaltered stack, composed of 129 linear frames combined in Nebulosity. This stack is available for download on the Nebula page. |
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The Curve function is used to begin expanding the thin histogram lines. The upper area of the curve is moved downward to prevent burning out highlights. In this image the function was applied 4 times to reach the desired brightness. The fuzzy edges caused by aligning 129 frames has been cropped. |
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The Levels function is now used to set the black point of the image. For each channel (red, green, blue) the left slider is moved to the right, stopping just before the spike. In addition, the red channel midpoint slider is moved slightly to the left (input level 1.25) to enhance the red just a little. The background is now neutral, and faint traces of the nebula can be seen. |
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At his point, two of Noel Carboni's Photoshop Action tools are employed:
Horizontal Banding Noise Reduction and Vertical Banding Noise Reduction. This reduces faint red lines which show up in my images, resulting from long exposures at ISO 1600. Some cameras don't produce such noise. Some produce even more. Longer exposures make it worse. The effect of these reduction tools is not visible in the small images used in this example, so I didn't display them. |
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Another application of the Curves function as in the first step above further expands the histogram. |
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The Levels function was used to set the black point (re-darkening the sky) and to further stretch the histogram. The adjustments are shown for each color channel, note the positions of the sliders for each channel. Now the detail is starting to come out. Compare this histogram with the one for the unaltered stack (scroll over it to see the original): |
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| Close examination of the image pixels reveals more noise has crept back in. The noise is faint and hard to see, but if not removed it will intensify as processing continues. Two of Carboni's Action Tools were applied: |
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Levels was used to reduce background brightness. |
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Again with Curves, the histogram is |
Photoshop's Saturation function was applied next. RGB channel+20. |
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Curves was used to brighten the midtones. Note the input level = 12. This prevents the background from lightening too much. |
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Carboni's Make Stars Smaller was applied three times. This tool must be used with care as it can produce odd background noise. |
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A final Curve adjustment and the image is done. This is by no means a perfect image. Longer exposures would have given much smoother results. This example was chosen to demonstrate how to get an image from underexposed raw files. |
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