TheoSSA - Theoretical Stellar Spectra Accesstheossa.raw_dataivo://org.gavo.dc/theossa/q/raw_dataThe GAVO DC teamRauch, T.2022-01-13T13:38:11ZThomas 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.https://dc.zah.uni-heidelberg.de/tableinfo/theossa.raw_dataArchiveSimulationOpticalUVtheossaTheoSSA - Theoretical Stellar Spectra AccessTheoSSA 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.
theossa.raw_dataTheoSSA 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.accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexedprimaryownerOwner of the datacharnullableembargoDate the data will become/became publicacharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Sizelongnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectioncharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablet_effEffective temperature assumedKphys.temperature.effectivefloatnullablelog_gLog of surface gravity assumedcm/s**2phys.gravityfloatnullablemdotMass loss ratesolMass/yrphys.mass.lossfloatnullablew_hMass fraction of H in the model computed.phys.abundfloatnullablew_heMass fraction of He in the model computed.phys.abundfloatnullablew_liMass fraction of Li in the model computed.phys.abundfloatnullablew_beMass fraction of Be in the model computed.phys.abundfloatnullablew_bMass fraction of B in the model computed.phys.abundfloatnullablew_cMass fraction of C in the model computed.phys.abundfloatnullablew_nMass fraction of N in the model computed.phys.abundfloatnullablew_oMass fraction of O in the model computed.phys.abundfloatnullablew_fMass fraction of F in the model computed.phys.abundfloatnullablew_neMass fraction of Ne in the model computed.phys.abundfloatnullablew_naMass fraction of Na in the model computed.phys.abundfloatnullablew_mgMass fraction of Mg in the model computed.phys.abundfloatnullablew_alMass fraction of Al in the model computed.phys.abundfloatnullablew_siMass fraction of Si in the model computed.phys.abundfloatnullablew_pMass fraction of P in the model computed.phys.abundfloatnullablew_sMass fraction of S in the model computed.phys.abundfloatnullablew_clMass fraction of Cl in the model computed.phys.abundfloatnullablew_arMass fraction of Ar in the model computed.phys.abundfloatnullablew_kMass fraction of K in the model computed.phys.abundfloatnullablew_caMass fraction of Ca in the model computed.phys.abundfloatnullablew_scMass fraction of Sc in the model computed.phys.abundfloatnullablew_tiMass fraction of Ti in the model computed.phys.abundfloatnullablew_vMass fraction of V in the model computed.phys.abundfloatnullablew_crMass fraction of Cr in the model computed.phys.abundfloatnullablew_mnMass fraction of Mn in the model computed.phys.abundfloatnullablew_feMass fraction of Fe in the model computed.phys.abundfloatnullablew_coMass fraction of Co in the model computed.phys.abundfloatnullablew_niMass fraction of Ni in the model computed.phys.abundfloatnullablew_znMass fraction of Zn in the model computed.phys.abundfloatnullablew_gaMass fraction of Ga in the model computed.phys.abundfloatnullablew_geMass fraction of Ge in the model computed.phys.abundfloatnullablew_krMass fraction of Kr in the model computed.phys.abundfloatnullablew_moMass fraction of Mo in the model computed.phys.abundfloatnullablew_tcMass fraction of Tc in the model computed.phys.abundfloatnullablew_snMass fraction of Sn in the model computed.phys.abundfloatnullablew_xeMass fraction of Xe in the model computed.phys.abundfloatnullablew_baMass fraction of Ba in the model computed.phys.abundfloatnullable