Difference between revisions of "Documentation/Nightly/Modules/AstroSmoothing"
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{{documentation/{{documentation/version}}/module-section|References}} | {{documentation/{{documentation/version}}/module-section|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} | ||
+ | } | ||
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Revision as of 08:38, 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
Tutorials
- Coming soon...
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}
}