Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-23T02:48:56.446Z Has data issue: false hasContentIssue false
  • English
  • Français

VO-KOREL: A Fourier Disentangling Service of the Virtual Observatory

Published online by Cambridge University Press:  23 April 2012

Petr Škoda ,
Petr Hadrava  and
Jan Fuchs
Petr Škoda
Affiliation:
Astronomical Institute, Academy of Sciences, Fričova 298, CZ-251 65 Ondřejov, Czech Republic email: [email protected]
Petr Hadrava
Affiliation:
Astronomical Institute, Academy of Sciences, Fričova 298, CZ-251 65 Ondřejov, Czech Republic email: [email protected]
Jan Fuchs
Affiliation:
Astronomical Institute, Academy of Sciences, Fričova 298, CZ-251 65 Ondřejov, Czech Republic email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

VO-KOREL is a web service exploiting the technology of the Virtual Observatory for providing astronomers with the intuitive graphical front-end and distributed computing back-end running the most recent version of the Fourier disentangling code KOREL.

The system integrates the ideas of the e-shop basket, conserving the privacy of every user by transfer encryption and access authentication, with features of laboratory notebook, allowing the easy housekeeping of both input parameters and final results, as well as it explores a newly emerging technology of cloud computing.

While the web-based front-end allows the user to submit data and parameter files, edit parameters, manage a job list, resubmit or cancel running jobs and mainly watching the text and graphical results of a disentangling process, the main part of the back-end is a simple job queue submission system executing in parallel multiple instances of the FORTRAN code KOREL. This may be easily extended for GRID-based deployment on massively parallel computing clusters.

The short introduction into underlying technologies is given, briefly mentioning advantages as well as bottlenecks of the design used.

Keywords

Methods: data analysistechniques: spectroscopicline:profilesVirtual Observatory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 403 - 404
Copyright
Copyright © International Astronomical Union 2012

References

Fielding, R. T. 2000, Architectural Styles and the Design of Network-based Software Architectures, Ph.D. Dissertation, University of California, Irvine, retrieved from http://www.ics.uci.edu/~fielding/pubs/dissertation/rest_arch_style.htmGoogle Scholar
Foster, I., Zhao, Y., Raicu, I., & Lu, S. 2008, Cloud Computing and Grid Computing 360-Degree Compared, arXiv:0901.0131CrossRefGoogle Scholar
Hadrava, P. 2009, Disentangling of spectra — theory and practice, arXiv:0909.0172CrossRefGoogle Scholar
Harrison, P. & Rixon, G. 2010, Universal Worker Service Pattern Version 1.0, IVOA Recommendation, retrieved from http://ivoa.net/Documents/UWS/index.htmlGoogle Scholar
Solano, E. 2006, Lecture Notes and Essays in Astrophysics, 2, 71Google Scholar