Documentation/Nightly/Modules/AstroModeling

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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 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 edit the value of 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{2017arXiv170306651P,
   author = {{Punzo}, D. and {van der Hulst}, J.~M. and {Roerdink}, J.~B.~T.~M. and 
	{Fillion-Robin}, J.~C. and {Yu}, L.},
    title = "{SlicerAstro: a 3-D interactive visual analytics tool for HI data}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1703.06651},
 primaryClass = "astro-ph.IM",
 keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
     year = 2017,
    month = mar,
   adsurl = {http://adsabs.harvard.edu/abs/2017arXiv170306651P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@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}
}