In the last decade, numerous Virtual Observatory organizations were established. One of these is the German Astrophysical Virtual Observatory (GAVO) that e.g. provides access to spectral energy distributions via the service TheoSSA. In a pilot phase, these are based on the Tuebingen NLTE Model-Atmosphere Package (TMAP) and suitable for hot, compact stars. We demonstrate the power of TheoSSA in an application to the sdOB primary of AA Doradus by comparison with a "classical" spectral analysis.
@article{arxiv.1111.0546,
title = {Spectral Analysis within the Virtual Observatory: The GAVO Service TheoSSA},
author = {Ellen Ringat},
journal= {arXiv preprint arXiv:1111.0546},
year = {2011}
}
Comments
Proceedings of sdOB5: The Fifth Meeting on Hot Subdwarf Stars & Related Objects, 10 pages, 9 figures