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Access to Stellar Population Models in the Virtual Observatory

Published online by Cambridge University Press:  01 December 2006

Igor V. Chilingarian
Igor V. Chilingarian*
Affiliation:
Sternberg Astronomical Institute, Moscow State University, 13 Universitetsky prospect, Moscow, 119992, Russia; email: [email protected] Centre de Recherche Astronomique de Lyon, Observatoire de Lyon, 9 Av. Charles André, Saint-Genis Laval, F-69561, France; CNRS, UMR 5574; Observatoire de Paris, LERMA, 61 Ave. de l'Observatoire, Paris, 75014, France
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Abstract

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A great effort is being made by the international Virtual Observatory community to build tools ready to be used by scientists. Presently, providing access to theoretical spectra in general, and synthetic spectra of galaxies in particular, is a matter of current interest in the Virtual Observatory. Several ways of accessing such spectra are available. We present two of them for accessing PEGASE.HR evolutionary synthesis models: HTTP-access to a limited number of parameters using Simple Spectral Access Protocol (SSAP), and full-featured WEB-service based access using Common Execution Architecture (CEA).

Keywords

astronomical data bases: miscellaneoustechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 177 - 178
Copyright
Copyright © International Astronomical Union 2007

References

LeBorgne, D. Borgne, D. et al. 2004, A&A 425, 881Google Scholar
Simon, G. et al. 2006, Proceedings of ADASS-XV, ASP Conference Series v. 351, 394Google Scholar
Tody, D. et al. 2006, SSAP v0.97, IVOA Working DraftGoogle Scholar