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<ri:Resource created="2024-08-09T08:06:16Z" 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>T4 APT photometry of HD 166620</title><shortName>J/ApJ/936/L23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/936/L23</identifier><altIdentifier>doi:10.26093/cds/vizier.19369023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luhn J.K.</name></creator><creator><name>Wright J.T.</name></creator><creator><name>Henry G.W.</name></creator><creator><name>Saar S.H.</name></creator><creator><name>Baum A.C.</name></creator><date role="Updated">2024-11-06T20:27:33Z</date><date role="Created">2024-08-09T08:06:16Z</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>high-velocity-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>HD-166620 was recently identified as a Maunder minimum candidate based on nearly 50 years of CaII H and K activity data from Mount Wilson and Keck HIRES. These data showed clear cyclic behavior on a 17yr timescale during the Mount Wilson survey that became flat when picked up later with Keck HIRES planet-search observations. Unfortunately, the transition between these two data sets-and therefore the transition into the candidate Maunder minimum phase-contained little to no data. Here, we present additional Mount Wilson data not present in Baum et al., along with photometry over a nearly 30yr baseline that definitively traces the transition from cyclic activity to a prolonged phase of flat activity. We present this as conclusive evidence of the star entering a grand magnetic minimum and therefore the first true Maunder minimum analog. We further show that neither the overall brightness nor the chromospheric activity level (as measured by SHK) is significantly lower during the grand magnetic minimum than its activity cycle minimum, implying that an anomalously low mean or instantaneous activity levels are not a good diagnostic or criterion for identifying additional Maunder minimum candidates. Intraseasonal variability in SHK, however, is lower in the star's grand minimum; this may prove a useful symptom of the phenomenon.</description><source format="bibcode">2022ApJ...936L..23L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/936/L23</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/AJ/111/439">J/AJ/111/439 : Chromospheric emission in late-type stars. (Henry+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/417/651">J/A+A/417/651 : NEXXUS ROSAT survey of coronal X-ray (Schmitt+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/152/261">J/ApJS/152/261 : Chromospheric Ca II emission in nearby stars (Wright+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/875">J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/32">J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/874/107">J/ApJ/874/107 : HARPS-N solar radial velocities &amp; activity (Milbourne+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/904/140">J/ApJ/904/140 : Ruprecht147 members &amp; rot. data 5 other cl. (Curtis+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/183">J/AJ/163/183 : S-value for 59 Sun-like starswith HIRES and HKP (Baum+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/180">J/AJ/163/180 : RVel &amp; BV photometry of 9 {gamma} Doradus stars (Henry+, 2022)</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/ApJ/936/L23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/936/L23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/936/L23</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/936/L23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/936/L23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/936/L23</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"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/936/L23/table2</name><description>All SHK activity data</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>JD</name><description>[2439342/2458918] Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Year</name><description>[1966/2021] Fractional year</description><unit>yr</unit><ucd>time</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SHK</name><description>[0.14/0.88] The S_HK_ activity index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Inst</name><description>Instrument identifier (1)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table><table><name>J/ApJ/936/L23/table3</name><description>T4 APT photometry</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>JD</name><description>[2449094/2459156] Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Year</name><description>[1993/2021] Fractional year</description><unit>yr</unit><ucd>time</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag</name><description>[0.76/0.78] Differential magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Inst</name><description>Instrument identifier (2)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>