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<ri:Resource created="2025-07-08T15:57:43Z" status="active" updated="2025-08-01T08:20:05Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.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:CatalogService"><title>Equivalent widths, Li &amp; activity for solar analogs</title><shortName>J/AJ/168/240</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/240</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lubin D.</name></creator><creator><name>Holden B.P.</name></creator><creator><name>Stock C.</name></creator><creator><name>Melis C.</name></creator><creator><name>Tytler D.</name></creator><date role="Updated">2025-08-01T08:20:05Z</date><date role="Created">2025-07-08T15:57:43Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>g-stars</subject><subject>line-intensities</subject><subject>chemical-abundances</subject><description>We measured lithium (Li) abundance and instantaneous chromospheric Ca_II_ HK activity in Hamilton Echelle Spectrograph observations of 211 solar analog field stars, with one objective being potential identification of grand minimum candidates for ongoing multiyear observation. At the zero-age main sequence, Li abundance for a typical late-type dwarf begins at the local interstellar medium abundance and over the main sequence lifetime is steadily depleted by convection at a rate dependent on details of the star's convection and mixing processes. Our Li abundance measurements show an overall decrease in Li abundance with age and effective temperature, consistent with earlier surveys. In our activity measurements, 41 stars show logR'_HK_&lt;=-5.0, which can be considered very inactive. Of the very inactive stars closest to solar effective temperature, 24 show Li abundances within the range typically observed for midlife Sun-like stars. Another three show very low Li abundance, which, combined with the low activity, suggest an older main sequence star or a slightly evolved star. We suggest that the combination of relatively undepleted Li and instantaneous very low activity might make these stars promising candidates for long time-series observations to determine if they are in a grand minimum state. The Hamilton Echelle Spectrograph observations are publicly available for download and are potentially useful for a variety of survey tasks involving Sun-like stars.</description><source format="bibcode">2024AJ....168..240L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/240</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/III/159">III/159 : Ca II H and K Measurements Made at MWO (Duncan+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/1059">J/AJ/106/1059 : Lithium in the Pleiades (Soderblom+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/111/439">J/AJ/111/439 : Chromospheric emission in late-type stars. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HD</name><description>[804/224465] HD identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Date</name><description>Date of Lick observation (1)</description><unit>'Y:M:D'</unit><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>ageEP</name><description>[1.24/10.1] Expectation age from Casagrande+ 2015, J/A+A/530/A138</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>C05</name><description>Display data from Casagrande+ 2005, J/A+A/530/A138 within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>S</name><description>[0.13/0.59] S units (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logRHK</name><description>[-5.2/-4.1] Log(R'_HK_) activity index (3)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EWLi</name><description>[3.8/118]? Equivalent width of Li 6708{AA} line, W_{lambda}_(Li) in m{AA}</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_logNLi</name><description>Upper limit flag on logNli</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logNLi</name><description>[0.4/3] Li abundance as Log(N_Li_)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EWbl</name><description>[0/15]? 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