<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2024-10-29T12:45:54Z" status="active" updated="2025-01-14T08:49:39Z" 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>CHIANTI Lines in LineTAP</title><shortName>chianti.lines</shortName><identifier>ivo://org.gavo.dc/chianti/q/lines</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Dere, K.</name></creator><creator><name>Mason, H.</name></creator><creator><name>Monsignori-Fossi, B.</name></creator><creator><name>Landi, E.</name></creator><creator><name>Young, P.</name></creator><creator><name>Landini, M.</name></creator><creator><name>Pike, D.</name></creator><creator><name>Bromage, G.</name></creator><creator><name>Bromage, B.</name></creator><creator><name>Del Zanna G.</name></creator><creator><name>Phillips, K.J.H.</name></creator><date role="Updated">2025-07-16T08:42:32Z</date><version>10.1</version><contact><name>GAVO Data Centre Team</name><address>Mönchhofstrasse 12-14, D-69120 Heidelberg</address><email>gavo@ari.uni-heidelberg.de</email><telephone>+49 6221 54 1837</telephone></contact></curation><content><subject>atomic-spectroscopy</subject><subject>line-positions</subject><description> CHIANTI consists of a critically evaluated set of up-to-date atomic
data and derived spectral lines.     At
http://www.chiantidatabase.org/, many tools for this data set are
available.  The present resource only takes the line data and makes it
available in standard LineTAP.

This is the state as of CHIANTI 10.1.</description><source format="bibcode">2023ApJS..268...52D</source><referenceURL>http://dc.g-vo.org/tableinfo/chianti.lines</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://org.gavo.dc/tap">GAVO Data Center TAP service</relatedResource></relationship></content><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface role="std" version="1.1" xsi:type="vs:ParamHTTP"><accessURL use="full">http://dc.g-vo.org/tap</accessURL><mirrorURL>https://dc.g-vo.org/tap</mirrorURL></interface></capability><coverage><spectral>1.986445857e-23 3.366286828e-15</spectral><waveband>Infrared</waveband><waveband>Optical</waveband><waveband>UV</waveband><waveband>EUV</waveband><waveband>X-Ray</waveband></coverage><tableset><schema><name>chianti</name><title>CHIANTI Lines in LineTAP</title><description> CHIANTI consists of a critically evaluated set of up-to-date atomic
data and derived spectral lines.     At
http://www.chiantidatabase.org/, many tools for this data set are
available.  The present resource only takes the line data and makes it
available in standard LineTAP.

This is the state as of CHIANTI 10.1.</description><table><name>chianti.lines</name><description> CHIANTI consists of a critically evaluated set of up-to-date atomic
data and derived spectral lines.     At
http://www.chiantidatabase.org/, many tools for this data set are
available.  The present resource only takes the line data and makes it
available in standard LineTAP.

This is the state as of CHIANTI 10.1.</description><utype>ivo://ivoa.net/std/linetap#lines-1.0</utype><nrows>2200000</nrows><column><name>title</name><description>Human-readable line designation.</description><ucd>meta.id</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>vacuum_wavelength</name><description>Vacuum wavelength of the transition</description><unit>Angstrom</unit><ucd>em.wl</ucd><stats><min>0.5901</min><percentile03>6.1778</percentile03><median>165.604</median><percentile97>2999.73</percentile97><max>1e+08</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>vacuum_wavelength_error</name><description>Total error in vacuum_wavelength</description><unit>Angstrom</unit><ucd>stat.error;em.wl</ucd><stats><fillFactor>0</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>method</name><description>Method the wavelength was obtained with (XSAMS controlled vocabulary)</description><ucd>meta.code.class</ucd><stats><option>observed</option><option>theory</option><option>ritz</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>element</name><description>Element name for atomic transitions, NULL otherwise.</description><ucd>phys.atmol.element</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ion_charge</name><description>Total charge (ionisation level) of the emitting particle.</description><ucd>phys.electCharge</ucd><stats><min>0</min><percentile03>2.0</percentile03><median>11.0</median><percentile97>24.0</percentile97><max>28</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType><flag>indexed</flag></column><column><name>mass_number</name><description>Number of nucleons in the atom or molecule</description><ucd>phys.atmol.weight</ucd><stats><fillFactor>0.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>upper_energy</name><description>Energy of the upper state</description><unit>J</unit><ucd>phys.energy;phys.atmol.initial</ucd><stats><min>3.26115e-22</min><percentile03>7.94895e-18</percentile03><median>8.17621e-17</median><percentile97>1.53852e-15</percentile97><max>3.36628e-15</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lower_energy</name><description>Energy of the lower state</description><unit>J</unit><ucd>phys.energy;phys.atmol.final</ucd><stats><min>0</min><percentile03>1.13668e-18</percentile03><median>5.49717e-17</median><percentile97>1.25788e-15</percentile97><max>3.35751e-15</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>inchi</name><description>International Chemical Identifier InChI.</description><ucd>meta.id;phys.atmol;meta.main</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag></column><column><name>inchikey</name><description>The InChi key (hash) generated from inchi.</description><ucd>meta.id;phys.atmol</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag></column><column><name>einstein_a</name><description>Einstein A coefficient of the radiative transition.</description><ucd>phys.atmol.transProb</ucd><stats><min>1e-30</min><percentile03>73502.8</percentile03><median>8.52e+07</median><percentile97>2.81e+11</percentile97><max>1.63e+15</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>xsams_uri</name><description>A URI for a full XSAMS description of this line.</description><ucd>meta.ref</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>line_reference</name><description>Reference to the source of the line data; this could be a bibcode, a DOI, or a plain URI.</description><ucd>meta.ref</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column></table></schema></tableset></ri:Resource>