tmap_webivo://org.gavo.dc/theossa/q/webThe 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.475.3896Rhttp://dc.g-vo.org/theossa/q/web/infoArchiveSimulationIsDerivedFromTMAWIsServedByGAVO Data Center ObscoreGAVO Data Center TAP service 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."http://dc.g-vo.org/theossahttps://dc.g-vo.org/theossahttp://dc.g-vo.org/theossa/q/web/capabilitieshttps://dc.g-vo.org/theossa/q/web/capabilitieshttp://dc.g-vo.org/theossa/q/web/availabilityhttps://dc.g-vo.org/theossa/q/web/availabilityhttp://dc.g-vo.org/theossa/q/web/tableMetadatahttps://dc.g-vo.org/theossa/q/web/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/taphttp://dc.g-vo.org/theossa/q/sdl/dlgethttps://dc.g-vo.org/theossa/q/sdl/dlgethttp://dc.g-vo.org/theossa/q/sdl/dlmetahttps://dc.g-vo.org/theossa/q/sdl/dlmetaGETapplication/x-votable+xml;content=datalinkIDThe publisher DID of the dataset of interestmeta.id;meta.maincharresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integerOpticalUVtheossaTheoSSA 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.outputTheoSSA 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.ssa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectioncharnullableaccrefAccess key for the datameta.ref.url;meta.datasetssa:Access.Referencecharnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start1e-102e-101.15005e-073.0005e-075.00106e-071floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop5.99979e-091.188e-071.78e-074e-054e-051floatnullablet_effEffective temperature assumedKphys.temperature.effective181003300059500940001.05e+061floatnullablelog_gLog of surface gravity assumedcm/s**2phys.gravity3.84.185.77.369.221floatnullablemdotMass loss ratesolMass/yrphys.mass.loss000001floatnullablew_hMass fraction of H in the model computed.phys.abund00.058910.5434111floatnullablew_heMass fraction of He in the model computed.phys.abund000.45420.937611floatnullablew_cMass fraction of C in the model computed.phys.abund000.0023910.0035250.59011floatnullablew_nMass fraction of N in the model computed.phys.abund00000.044061floatnullablew_oMass fraction of O in the model computed.phys.abund00000.69431floatnullablew_fMass fraction of F in the model computed.phys.abund00000.00010.999472floatnullablew_naMass fraction of Na in the model computed.phys.abund00000.0099010.999379floatnullablew_mgMass fraction of Mg in the model computed.phys.abund00000.093820.999501floatnullablew_alMass fraction of Al in the model computed.phys.abund00000.0099011floatnullablew_siMass fraction of Si in the model computed.phys.abund00000.019261floatnullablew_pMass fraction of P in the model computed.phys.abund00003.172e-050.99996floatnullablew_sMass fraction of S in the model computed.phys.abund00000.0030831floatnullablew_clMass fraction of Cl in the model computed.phys.abund00004.943e-060.999196floatnullablew_arMass fraction of Ar in the model computed.phys.abund00000.00013990.999472floatnullablew_caMass fraction of Ca in the model computed.phys.abund00000.0063591floatnullablew_feMass fraction of Fe in the model computed.phys.abund00000.012920.99996floatnullablew_coMass fraction of Co in the model computed.phys.abund00000.00087150.999415floatnullablew_niMass fraction of Ni in the model computed.phys.abund00000.007050.999859floatnullablew_geMass fraction of Ge in the model computed.phys.abund00000.00023991floatnullablew_krMass fraction of Kr in the model computed.phys.abund00000.0010991floatnullablew_snMass fraction of Sn in the model computed.phys.abund00000.00020361floatnullablew_xeMass fraction of Xe in the model computed.phys.abund00000.0016971floatnullablew_znMass fraction of Zn in the model computed.phys.abund00000.000171floatnullablew_baMass fraction of Ba in the model computed.phys.abund00000.0014981floatnullable