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Fast Algorithms for Matching CCD Images to a Stellar Catalogue

V. Tabur

School of Physics A28, University of Sydney, NSW 2006, Australia. Email: tabur@physics.usyd.edu.au


Abstract

Two new algorithms are described for matching two dimensional coordinate lists of point sources that are significantly faster than previous methods. By matching rarely occurring triangles (or more complex shapes) in the two lists, and by ordering searches by decreasing probability of success, it is demonstrated that very few candidates need be considered to find a successful match. Moreover, by immediately testing the suitability of a potential match using an efficient mechanism, the need to process the entire candidate set is avoided, yielding considerable performance improvements. Triangles are described by a cosine metric that reduces the density of triangle space, permitting efficient searches. An alternative shape characterization method that reduces computational overhead in the construction phase is discussed. The algorithms are tested on a set of 10 063 wide-field survey images, with fields-of-view up to 4.8° × 3.6°, successfully matching 100% of the images in a mean elapsed time of 6 ms (2.4 GHz Athlon CPU). The elapsed time of the searching phase is shown to vary by less than 1ms for list sizes between 10 and 200 points, demonstrating that fast, robust searches may be completed in nearly constant time, independent of list size.

Keywords: astrometry — methods: data analysis — surveys

Publications of the Astronomical Society of Australia 24(4) 189–198    doi:10.1071/AS07028
Submitted: 13 August 2007    Accepted: 16 October 2007    Published: 7 December 2007





   
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