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New Algorithms for Automated Astrometry

Chris Harvey-2004-01-01-TSpace

TL;DRAbstract

In the second approach we search an image for constrained n-star shapes and match them to similar shapes in a pre-computed table. We show that by using constrained shapes we can reduce the time to match n-star shapes to the order of matching arbitrary 4-star shapes. Finally, we perform experiments on synthetic and real catalogs and show that both approaches perform well. In the 'lost-in-space' astronomy problem we are asked to identify the orientation and field-of-view of an image of the sky by matching stars in an image to stars in a catalog. In this work we present two solutions to the problem. In the first approach we reduce an image to coarse positional information represented by a bit-string. We show that by making one assumption about the image we can efficiently solve the orientation problem using bitwise logical operations over an index.

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In the second approach we search an image for constrained n-star shapes and match them to similar shapes in a pre-computed table. We show that by using constrained shapes we can reduce the time to match n-star shapes to the order of matching arbitrary 4-star shapes. Finally, we perform experiments on synthetic and real catalogs and show that both approaches perform well. In the 'lost-in-space' astronomy problem we are asked to identify the orientation and field-of-view of an image of the sky by matching stars in an image to stars in a catalog. In this work we present two solutions to the problem. In the first approach we reduce an image to coarse positional information represented by a bit-string. We show that by making one assumption about the image we can efficiently solve the orientation problem using bitwise logical operations over an index.

Keywords

AstrometryComputer scienceAlgorithmArtificial intelligenceComputer visionStars

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