Difference between revisions of "Documentation/Nightly/Modules/AstroSmoothing"
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<b>Steve Pieper</b> (Isomics) <br> | <b>Steve Pieper</b> (Isomics) <br> | ||
+ | <b>Jean-Christophe Fillion-Robin</b> (Kitware) <br> | ||
+ | <b>Ken Martin</b> (Kitware) <br> | ||
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Revision as of 12:00, 14 September 2016
Home < Documentation < Nightly < Modules < AstroSmoothing
For the latest Slicer documentation, visit the read-the-docs. |
Introduction and Acknowledgements
Authors: Contributors: Acknowledgements: Contacts:
|
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{2016arXiv160903782P, author = {{Punzo}, D. and {van der Hulst}, J.~M. and {Roerdink}, J.~B.~T.~M. }, title = "{Finding faint HI structure in and around galaxies: scraping the barrel}", journal = {ArXiv e-prints}, archivePrefix = "arXiv", eprint = {1609.03782}, primaryClass = "astro-ph.IM", keywords = {Astrophysics - Instrumentation and Methods for Astrophysics}, year = 2016, month = sep, adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160903782P}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }