Inside Collection (Course): ELEC 301 Projects Fall 2006
Summary: Final results for astronomical image processing using Weiner filtering and weighted averaging.
The final estimation of the original object can be seen below; the black border on the left and bottom sides of the image was created by the image registration process. As shown in the image and below, the noise level of the image was greatly reduced. Also, the star points appear much more focused, and several stars that were previously very dim now appear more clearly in the processed image.
| Final Image |
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| Noise Variance |
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