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arXiv 1406.1528cs.CVastro-ph.IM

Towards building a Crowd-Sourced Sky Map

Carnegie Mellon University(卡内基梅隆大学);New York University(纽约大学);Max Planck Institute for Intelligent Systems(马克斯·普朗克智能系统研究所)

Dustin Lang, David W. Hogg, Bernhard Scholkopf

英文摘要:

We describe a system that builds a high dynamic-range and wide-angle image of the night sky by combining a large set of input images. The method makes use of pixel-rank information in the individual input images to improve a "consensus" pixel rank in the combined image. Because it only makes use of ranks and the complexity of the algorithm is linear in the number of images, the method is useful for large sets of uncalibrated images that might have undergone unknown non-linear tone mapping transformations for visualization or aesthetic reasons. We apply the method to images of the night sky (of unknown provenance) discovered on the Web. The method permits discovery of astronomical objects or features that are not visible in any of the input images taken individually. More importantly, however, it permits scientific exploitation of a huge source of astronomical images that would not be available to astronomical research without our automatic system.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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