Difference between revisions of "Documentation/Nightly/Modules/AstroModeling"

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[[File:ERCIcon.png|300px|European Research Council]]
 
[[File:Kapteyn logo1.png|500px|Kapteyn Astronomical Institute]]
 
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{{documentation/{{documentation/version}}/module-section|Introduction and Acknowledgements}}
 
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Authors:<br>
 
<b>Davide Punzo</b> (Kapteyn Astronomical Institute, University of Groningen) <br>
 
<b>Thijs van der Hulst</b> (Kapteyn Astronomical Institute, University of Groningen) <br>
 
<b>Jos Roerdink</b> (Johann Bernoulli Institute for Mathematics and Computer Science, University of Groningen) <br> <br>
 
  
Acknowledgements: <br>
 
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.<br> <br>
 
 
 
 
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>
 
[http://www.slicer.org/slicerWiki/index.php/Documentation/Nightly/Extensions/SlicerAstro Back to SlicerAstro home]
 
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{{documentation/{{documentation/version}}/module-section|Module Description}}
 
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>
 
In addition, SlicerAstro provides an easy and interactive interface for comparing the automated-generated models with the data. <br>
 
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. <br><br>
 
 
 
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* Select the Input: <br><br>
 
[[File:SlicerAstroWiki12.png|1000px]]
 
<br><br>
 
 
 
* Modify and Visualize the model: <br><br>
 
[[File:SlicerAstroWiki13.png|1000px]]
 
<br><br>
 
 
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{{documentation/{{documentation/version}}/module-section|References}}
 
 
<pre>
 
@ARTICLE{2017A&C....19...45P,
 
  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 = {Astronomy and Computing},
 
archivePrefix = "arXiv",
 
  eprint = {1703.06651},
 
primaryClass = "astro-ph.IM",
 
keywords = {Radio lines: galaxies, Scientific visualization, Visual analytics, Agile software development, Object oriented development, Empirical software validation},
 
    year = 2017,
 
    month = apr,
 
  volume = 19,
 
    pages = {45-59},
 
      doi = {10.1016/j.ascom.2017.03.004},
 
}
 
 
</pre>
 
<pre>
 
@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},
 
}
 
</pre>
 
 
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Revision as of 13:39, 10 December 2017

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