ivo://org.gavo.dc/theossa/q/sdlThe GAVO DC teamRauch, T.2026-01-20T07:42:29ZThomas Rauchgavo@listserv.uni-tuebingen.de++49 7071 2978614spectroscopyastronomical-simulationspost-asymptotic-giant-branch-starsstellar-atmospheresTheoSSA provides spectral energy distributions based on model atmosphere calculations. Currently, we serve results obtained using the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact stars.2018MNRAS.475.3896Rhttps://dc.g-vo.org/theossa/q/sdl/infoArchiveSimulation When publishing research making use of this service, please acknowledge: "The TheoSSA service (http://dc.g-vo.org/theossa) used to retrieve theoretical spectra for this paper was constructed as part of the activities of the German Astrophysical Virtual Observatory."OpticalUV