Difference between revisions of "Documentation/Nightly/Modules/AstroModeling"
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− | The Modeling module is a C++ SlicerAstro wrapping of 3DBAROLO [http://editeodoro.github.io/Bbarolo/]: a new 3D algorithm to derive rotation curves of galaxies. | + | The Modeling module is a C++ SlicerAstro wrapping of 3DBAROLO [http://editeodoro.github.io/Bbarolo/]: a new 3D algorithm to derive rotation curves of galaxies. <br> |
− | In addition, SlicerAstro provides an easy and interactive interface to comapre the generated models with the data | + | In addition, SlicerAstro provides an easy and interactive interface to comapre the generated models with the data <br> |
− | and change the parameters of such models to refine the analysis of the kinematics of a galaxy. | + | and change the parameters of such models to refine the analysis of the kinematics of a galaxy. <br><br> |
Revision as of 14:32, 22 November 2016
Home < Documentation < Nightly < Modules < AstroModeling
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Introduction and Acknowledgements
Authors: Acknowledgements:
Contacts:
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Module Description
The Modeling module is a C++ SlicerAstro wrapping of 3DBAROLO [1]: a new 3D algorithm to derive rotation curves of galaxies.
In addition, SlicerAstro provides an easy and interactive interface to comapre the generated models with the data
and change the parameters of such models to refine the analysis of the kinematics of a galaxy.
Panels and their use
References
@ARTICLE{2015MNRAS.451.3021D, author = {{Di Teodoro}, E.~M. and {Fraternali}, F.}, title = "{$^{3D}$ BAROLO: a new 3D algorithm to derive rotation curves of galaxies}", journal = {\mnras}, archivePrefix = "arXiv", eprint = {1505.07834}, keywords = {methods: data analysis, galaxies: kinematics and dynamics}, year = 2015, month = aug, volume = 451, pages = {3021-3033}, doi = {10.1093/mnras/stv1213}, adsurl = {http://adsabs.harvard.edu/abs/2015MNRAS.451.3021D}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }