UNSHARP MASKING OF DIGITAL ASTRONOMICAL IMAGES



The issue of Digital Masking in our AO images spurred a lot of discussion in S.A.A.. Rather than dealing with these individually we have chosen to add this page to our HINTS section.

We discussed Photographic Masking in great detail in AMOACP and will spend a lot of time on digital masking in our new book. This will show you a few basic highlights of the process. For those interested in the historical situation, David Malin adopted and used a process that was fine tuned to near perfection by Wm C. "Bill" Miller of Hale Observatories. Bill was a good friend and mentor!

Unsharp Masking allows one to reduce the overall large-scale contrast of an image while retaining the local contrast of small details within the images. Thus, one can reduce the brighness range between the bright nucleus of a galaxy and its faint outer spiral arms while preserving the local contrast showing dark lanes and bright globules throught the image of the galaxy.

While PhotoShop is great for 'normal' photographs, their masking routines are not well designed for use with astronomical images ( yet ). While a major improvement in masking capability occured in the move to PShop 3.0 ( and 4.0 ) this is still not totally suitable for astronomical images.


WHY DOESN'T THE PHOTOSHOP MASKING TOOL
WORK WELL ON ASTRONOMICAL IMAGES ?


Astronomical images contain stars. The normal blurring of the image to make a good mask for an astronomical image creates blurred stars. A good mask needs to show virtually NO residuals of these stars in the field and the perfect mask would show no sign of the stars. Any residuals traces of stars will produce characteristic 'black eyes' around stars when the negative mask and the original image are combined.

MIRA does a good job masking astronomical images. IDL allows one to build a filter that does an excellent job of removing the residuals from the star images. In PhotoShop, one can produce a very blurred image by repeated passes of their Gaussian Blur function and then remove the residuals using the 'Rubber Stamp' tool.

ORIGINAL IMAGE:



20 min exposure, ST-7 ( non-ABG) with No.25 RED filter
12.5-inch f/9 Ritchey ( with a very bad collimation problem ! )
Pseudo-color added using IDL 'temperature' color table 3

THE MASK:



At this point one has a choice of varying the degree of masking to achieve different effects.

THE FINAL IMAGE:


LIGHT MASKING:

MEDIUM MASKING:

MAXIMUM MASKING:




Enjoy !!

Brad Wallis
All work for these examples were performed using IDL.
All images are Copyright 1997 Brad D Wallis.

No Images from this web page or this web site may be used for any purposes without the express written consent of Brad D Wallis.
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