Difference between revisions of "Documentation/4.8/Modules/AstroSmoothing"
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* Thijs van der Hulst, <email>J.M.van.der.Hulst@astro.rug.nl</email> | * Thijs van der Hulst, <email>J.M.van.der.Hulst@astro.rug.nl</email> | ||
* Jos Roerdink <email>j.b.t.m.roerdink@rug.nl</email> | * Jos Roerdink <email>j.b.t.m.roerdink@rug.nl</email> | ||
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Latest revision as of 02:25, 27 November 2019
Home < Documentation < 4.8 < Modules < AstroSmoothing
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For the latest Slicer documentation, visit the read-the-docs. |
Introduction and Acknowledgements
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Authors: Contributors: Acknowledgements: Contacts:
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Module Description
The Smoothing module contain a set of filters (parallelized with OpenMP and OpenGL) aimed to denoise astronomical (HI) dataset:
- Anisotropic Box
- Anisotropic Gaussian
- Intensity-driven Gradient
Panels and their use
References
@ARTICLE{2016A&C....17..163P,
author = {{Punzo}, D. and {van der Hulst}, J.~M. and {Roerdink}, J.~B.~T.~M.
},
title = "{Finding faint H I structure in and around galaxies: Scraping the barrel}",
journal = {Astronomy and Computing},
archivePrefix = "arXiv",
eprint = {1609.03782},
primaryClass = "astro-ph.IM",
keywords = {Radio lines: galaxies, Techniques: image processing, Scientific visualization},
year = 2016,
month = oct,
volume = 17,
pages = {163-176},
doi = {10.1016/j.ascom.2016.09.002},
}