Home Page Sat Dec 6 19:31:03 JST 1997
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Star detection and noisesAs [2] says, matching process in the PIXY system consists of two steps, star detection from an image and then matching two sets of points, that of detected stars and star data in a catalog. Matching itself succeeds for many images as mentioned before. However the process of star detection is still preliminary and quite incomplete. I show you an example. This image is the plot of detected stars from the image of Comet Hyakutake (hy960327.jpg), a successful example in the previous section.
Among the sample images listed up in Section 2, the two: hb970117.jpg and hb970309b.jpg were failed to be matched. The reason in both cases is because many noises appeared in the flattening process and they were all recognized as faint stars. These images were taken in a morning or evening glow and the background level is very different depending on the position on the image. That is, the flattening method mentioned in [3] cannot be applied to them. So the flattening caused an adverse effect in both cases. However, there is a successful case of an image taken in a morning glow (hb970103.jpg). I do not know why matching sometimes succeeded and sometimes failed for such images.
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Next: Accuracy of matching Up: Interim Report on Matching Previous: Matching of peculiar images |