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ACM Computing Classification System (1998): I.2.8, I.2.10, I.5.1, J.2.
Given the coarse celestial coordinates of the centre of a plate
scan and the field of view, we are looking for a mapping between the stars
extracted from the image and the stars from a catalogue, where the stars
from both sources are represented by their stellar magnitudes and coordinates, relatively to the image centre. In a previous work we demonstrated
the application of Iterative Closest Point (ICP) algorithm...
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