Speaker
Dr
T. Rauch
Description
In the framework of the German Astrophysical Virtual Observatory (GAVO), several services and tools have been developed in the last two decades. This includes, e.g., the Theoretical Stellar Spectra Access (TheoSSA) service that provides synthetic stellar spectra calculated by the Tuebingen non-local thermodynamic equilibrium Model-Atmosphere Package (TMAP). About 500000 precalculated stellar energy distributions (SEDs) are presently available, individual SEDs will be calculated on demand. These may be used for precise spectral analyses of hot, compact stars, e.g., subdwarfs, white dwarfs, and even neutron stars.
