Institut für Astronomie und Astrophysik
Abteilung AstronomieSand 1, D-72076 Tübingen, Germany
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E. Ringat and T. Rauch
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics,
Eberhard Karls University, Sand 1, D-72076 Tübingen, Germany
To be published in: Proceedings of the 17th European White Dwarf Workshop, AIP Conference Series
Abstract. In the last decades, a lot of progress was made in spectral analysis. The quality (e.g. resolution, S/N ratio) of observed spectra has improved much and several model-atmosphere codes were developed. One of these is the Tübingen NLTE Model-Atmosphere Package (TMAP), that is a highly developed program for the calculation of model atmospheres of hot, compact objects.
In the framework of the German Astrophysical Virtual Observatory (GAVO), theoretical spectral energy distributions (SEDs) can be downloaded via TheoSSA. In a pilot phase, TheoSSA is based on TMAP model atmospheres.We present the current state of this VO service.
Preprint (202 kb PDF file including figures)
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Last modified 05 Oct 2010