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<ri:Resource created="2018-10-16T07:23:40Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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://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:CatalogService"><title>Line lists for X^1^{Sigma}^+^ AlF and AlCl</title><shortName>J/ApJS/237/8</shortName><identifier>ivo://CDS.VizieR/J/ApJS/237/8</identifier><altIdentifier>doi:10.26093/cds/vizier.22370008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yousefi M.</name></creator><creator><name>Bernath P.F.</name></creator><date role="Updated">2018-11-23T11:28:56Z</date><date role="Created">2018-10-16T07:23:40Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>atomic-physics</subject><subject>molecular-physics</subject><description>Vibration-rotation line lists for AlF, Al^35^Cl, and Al^37^Cl have been prepared in their ground electronic states (X^1^{Sigma}^+^). Experimental rotational and ro-vibrational lines were employed to calculate a potential energy surface (PES) by direct potential fitting. The PES was used to calculate ro-vibrational energy levels. Born-Oppenheimer Breakdown corrections were included in the energy level calculations for AlCl. Ro-vibrational energy levels were calculated for the v=0 to v=11 vibrational levels and up to Jmax=200 for the rotational levels. Dipole moment functions covering the range of the PES turning points were calculated for AlCl and AlF by ab initio methods and used to determine line intensities. Partition functions for temperatures up to 3000K were calculated. AlF and AlCl have been detected in circumstellar envelopes and are predicted to occur in cool stellar and sub- stellar atmospheres.</description><source format="bibcode">2018ApJS..237....8Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/237/8</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/442/1821">J/MNRAS/442/1821 : ExoMol line list for KCl (Barton+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/150">J/ApJ/825/150 : Laboratory spectroscopy of sodium chloride (Cabezas+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/8">J/ApJS/235/8 : Line lists for X^1^{Sigma}^+^ LiF and LiCl (Bittner+, 2018)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/237/8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/237/8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/237/8</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/237/8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/237/8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/237/8</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/ApJS/237/8/table2</name><description>Dipole moment functions for the X^1^{Sigma}^+^ states of AlF and AlCl in Debye</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>r</name><description>[1.2/2.7] Internuclear distance</description><unit>0.1nm</unit><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>AlF</name><description>[-4.2/0.3]? AlF Dipole moment</description><unit>D</unit><ucd>phys.mol.dipole</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>AlCl</name><description>[-4.9/0.5]? AlCl Dipole moment</description><unit>D</unit><ucd>phys.mol.dipole</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/237/8/table7</name><description>Line lists for AlF and AlCl in the X^1^{Sigma}^+^ ground state</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Iso</name><description>Isotopologue (Al35Cl, Al37Cl or AlF)</description><ucd>meta.id;phys.mol</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Branch</name><description>Branch (Lower J quantum number)</description><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>v1</name><description>[0/11] Upper vibrational quantum number</description><ucd>phys.atmol.qn;phys.mol.vibration;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>v0</name><description>[0/10] Lower vibrational quantum number</description><ucd>phys.atmol.qn;phys.mol.vibration;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ev0J0</name><description>[237.6/26595.6] Lower state energy</description><unit>cm**-1</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>v</name><description>[-3881.2/-0.4] Transition wavenumber</description><unit>cm**-1</unit><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>A</name><description>[3.3e-14/75.4] Einstein A coefficient</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f</name><description>[1e-20/0.0004] Oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDMMEs</name><description>[-3.2/0.2] Transition dipole moment matrix elements</description><unit>D</unit><ucd>phys.mol.dipole;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>