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.
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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. <br>
In addition, SlicerAstro provides an easy and interactive interface to comapre the generated models with the data
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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.
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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


For the latest Slicer documentation, visit the read-the-docs.


European Research Council Kapteyn Astronomical Institute

Introduction and Acknowledgements

Authors:
Davide Punzo (Kapteyn Astronomical Institute, University of Groningen)
Thijs van der Hulst (Kapteyn Astronomical Institute, University of Groningen)
Jos Roerdink (Johann Bernoulli Institute for Mathematics and Computer Science, University of Groningen)

Acknowledgements:
This work was supported by the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement nr. 291-531.


Contacts:

  • Davide Punzo, <email>punzodavide@hotmail.it</email>; <email>D.Punzo@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>

Back to SlicerAstro home

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

  • SlicerAstroWiki8.png


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}
}