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Cosmic‐Ray Rejection by Laplacian Edge Detection

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van Dokkum, Pieter G.·2001·Publications of the Astronomical Society of the Pacific

Abstract

Conventional algorithms for rejecting cosmic rays in single CCD exposures rely on the contrast between cosmic rays and their surroundings and may produce erroneous results if the point‐spread function is smaller than the largest cosmic rays. This paper describes a robust algorithm for cosmic‐ray rejection, based on a variation of Laplacian edge detection. The algorithm identifies cosmic rays of arbitrary shapes and sizes by the sharpness of their edges and reliably discriminates between poorly sampled point sources and cosmic rays. Examples of its performance are given for spectroscopic and imaging data, including Hubble Space Telescope Wide Field Planetary Camera 2 images.

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Metadata

Authors
van Dokkum, P. G.
Venue
Publications of the Astronomical Society of the Pacific
Published
2001-11
Volume
113
Issue
789
Pages
1420-1427
ISSN
  • 0004-6280 (ISSN-L)
  • 1538-3873
OpenAlex
W2102748875
Cited by
1,626
References
1
FWCI
14.64
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Cosmic‐Ray Rejection by Laplacian Edge Detection. https://app.cochat.ai/papers/10.1086/323894
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van Dokkum, P. G. (2001). Cosmic‐Ray Rejection by Laplacian Edge Detection. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/323894

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