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/], | + | The Modeling module is a C++ SlicerAstro wrapping of 3DBAROLO [http://editeodoro.github.io/Bbarolo/], |
a 3D algorithm to derive rotation curves of galaxies, developed by <b> Enrico di Teodoro </b> (Australian National University). <br> | a 3D algorithm to derive rotation curves of galaxies, developed by <b> Enrico di Teodoro </b> (Australian National University). <br> | ||
In addition, SlicerAstro provides an easy and interactive interface for comparing the automated-generated models with the data. <br> | In addition, SlicerAstro provides an easy and interactive interface for comparing the automated-generated models with the data. <br> |
Revision as of 16:56, 22 November 2016
Home < Documentation < Nightly < Modules < AstroModeling
For the latest Slicer documentation, visit the read-the-docs. |
Introduction and Acknowledgements
Authors: Acknowledgements:
Contacts:
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Module Description
The Modeling module is a C++ SlicerAstro wrapping of 3DBAROLO [1],
a 3D algorithm to derive rotation curves of galaxies, developed by Enrico di Teodoro (Australian National University).
In addition, SlicerAstro provides an easy and interactive interface for comparing the automated-generated models with the data.
It is also possible to change each parameter for each ring of the tilted-ring model for refining the analysis of the kinematics of the galaxy in study.
Panels and their use
- Select the Input:
- Modify and Visualize the model:
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} }