<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2010-11-11T15:00:00Z" status="active" updated="2026-01-20T07:14:45Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://dc.g-vo.org/ColStats-1 http://vo.ari.uni-heidelberg.de/docs/schemata/Colstats.xsd http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogResource"><title>TheoSSA - Theoretical Stellar Spectra Access</title><shortName>theossa.raw_data</shortName><identifier>ivo://org.gavo.dc/theossa/q/raw_data</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Rauch, T.</name></creator><date role="Updated">2026-01-20T07:42:29Z</date><contact><name>Thomas Rauch</name><email>gavo@listserv.uni-tuebingen.de</email><telephone>++49 7071 2978614</telephone></contact></curation><content><subject>spectroscopy</subject><subject>astronomical-simulations</subject><subject>post-asymptotic-giant-branch-stars</subject><subject>stellar-atmospheres</subject><description>TheoSSA 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.</description><source format="bibcode">2018MNRAS.475.3896R</source><referenceURL>https://dc.g-vo.org/tableinfo/theossa.raw_data</referenceURL><type>Archive</type><type>Simulation</type></content><coverage><waveband>Optical</waveband><waveband>UV</waveband></coverage><tableset><schema><name>theossa</name><title>TheoSSA - Theoretical Stellar Spectra Access</title><description>TheoSSA 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.</description><table><name>theossa.raw_data</name><description>TheoSSA 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.</description><nrows>2000000</nrows><column><name>accref</name><description>Access key for the data</description><ucd>meta.ref.url</ucd><utype>Access.Reference</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag><flag>primary</flag></column><column><name>owner</name><description>Owner of the data</description><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>embargo</name><description>Date the data will become/became public</description><unit>yr</unit><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>mime</name><description>MIME type of the file served</description><ucd>meta.code.mime</ucd><utype>Access.Format</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>accsize</name><description>Size of the data in bytes</description><unit>byte</unit><ucd>VOX:Image_FileSize</ucd><utype>Access.Size</utype><stats><min>6331</min><percentile03>69872.28</percentile03><median>126339.0</median><percentile97>1266903.88</percentile97><max>4203787</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>ssa_location</name><description>ICRS location of aperture center</description><unit>deg</unit><ucd>pos.eq</ucd><utype>ssa:Char.SpatialAxis.Coverage.Location.Value</utype><dataType arraysize="2" extendedType="point" xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ssa_dstitle</name><description>A compact and descriptive designation of the dataset.</description><ucd>meta.title;meta.dataset</ucd><utype>ssa:DataID.Title</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>ssa_creatordid</name><description>Dataset identifier assigned by the creator</description><ucd>meta.id</ucd><utype>ssa:DataID.CreatorDID</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_cdate</name><description>Processing/Creation date</description><ucd>time;meta.dataset</ucd><utype>ssa:DataID.Date</utype><stats><min>52045.00212962963</min><percentile03>56675.478738425925</percentile03><median>59691.77164351852</median><percentile97>60691.701585648145</percentile97><max>60722.48752314815</max><fillFactor>1.0</fillFactor></stats><dataType arraysize="19" extendedType="timestamp" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_pdate</name><description>Date last published.</description><utype>ssa:Curation.Date</utype><stats><min>59592.543115186374</min><percentile03>59592.547566521294</percentile03><median>60779.676765362754</median><percentile97>61060.320205364034</percentile97><max>61090.55185453736</max><fillFactor>1.0</fillFactor></stats><dataType arraysize="19" extendedType="timestamp" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_cversion</name><description>Creator assigned version for this dataset (will be incremented when this particular item is changed).</description><ucd>meta.version;meta.dataset</ucd><utype>ssa:DataID.Version</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_targname</name><description>Common name of object observed.</description><ucd>meta.id;src</ucd><utype>ssa:Target.Name</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag></column><column><name>ssa_redshift</name><description>Redshift of target object</description><ucd>src.redshift</ucd><utype>ssa:Target.Redshift</utype><stats><fillFactor>0</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_aperture</name><description>Angular diameter of aperture</description><unit>deg</unit><ucd>phys.angSize;instr.fov</ucd><utype>ssa:Char.SpatialAxis.Coverage.Bounds.Extent</utype><stats><min>0.0001</min><percentile03>0.0001</percentile03><median>0.0001</median><percentile97>0.0001</percentile97><max>0.0001</max><fillFactor>3.85279e-05</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_specstart</name><description>Lower value of spectral coordinate</description><unit>m</unit><ucd>em.wl;stat.min</ucd><utype>ssa:Char.SpectralAxis.Coverage.Bounds.Start</utype><stats><min>1e-10</min><percentile03>2e-10</percentile03><median>1.15005e-07</median><percentile97>3.0005e-07</percentile97><max>5.00106e-07</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ssa_specend</name><description>Upper value of spectral coordinate</description><unit>m</unit><ucd>em.wl;stat.max</ucd><utype>ssa:Char.SpectralAxis.Coverage.Bounds.Stop</utype><stats><min>5.99979e-09</min><percentile03>1.188e-07</percentile03><median>1.78e-07</median><percentile97>4e-05</percentile97><max>4e-05</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ssa_length</name><description>Number of points in the spectrum</description><utype>ssa:Dataset.Length</utype><stats><min>912</min><percentile03>7679.0</percentile03><median>14723.0</median><percentile97>173663.0</percentile97><max>686196</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ssa_creator</name><description>Creator of the datasets included here.</description><utype>ssa:DataID.Creator</utype><dataType arraysize="*" xsi:type="vs:VOTableType">unicodeChar</dataType><flag>nullable</flag></column><column><name>ssa_collection</name><description>A short handle naming the collection this spectrum belongs to.</description><utype>ssa:DataID.Collection</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_instrument</name><description>Instrument or code used to produce these datasets</description><ucd>meta.id;instr</ucd><utype>ssa:DataID.Instrument</utype><dataType arraysize="*" 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_he</name><description>Mass fraction of He in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0.4542</median><percentile97>0.9376</percentile97><max>1</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_li</name><description>Mass fraction of Li in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0</max><fillFactor>0.999196</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_be</name><description>Mass fraction of Be in the model 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_mg</name><description>Mass fraction of Mg in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.09382</max><fillFactor>0.999501</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_al</name><description>Mass fraction of Al in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.009901</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_si</name><description>Mass fraction of Si in the model 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_cl</name><description>Mass fraction of Cl in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>4.943e-06</max><fillFactor>0.999196</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_ar</name><description>Mass fraction of Ar in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.0001399</max><fillFactor>0.999472</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_k</name><description>Mass fraction of K in the model 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_ti</name><description>Mass fraction of Ti in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.00309</max><fillFactor>0.999362</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_v</name><description>Mass fraction of V in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>5.675e-09</max><fillFactor>0.999196</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_cr</name><description>Mass fraction of Cr in the model 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_co</name><description>Mass fraction of Co in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.0008715</max><fillFactor>0.999415</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_ni</name><description>Mass fraction of Ni in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.00705</max><fillFactor>0.999859</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_zn</name><description>Mass fraction of Zn in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.00017</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_ga</name><description>Mass fraction of Ga in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.0005597</max><fillFactor>0.865835</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_ge</name><description>Mass fraction of Ge in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.0002399</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_kr</name><description>Mass fraction of Kr in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.001099</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_mo</name><description>Mass fraction of Mo in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.0001881</max><fillFactor>0.86563</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_tc</name><description>Mass fraction of Tc in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0</max><fillFactor>0.865142</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_sn</name><description>Mass fraction of Sn in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.0002036</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_xe</name><description>Mass fraction of Xe in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.001697</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>w_ba</name><description>Mass fraction of Ba in the model computed.</description><ucd>phys.abund</ucd><stats><min>0</min><percentile03>0</percentile03><median>0</median><percentile97>0</percentile97><max>0.001498</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>