<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2016-02-22T13:07:12Z" 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>S-index and Stroemgren LC of HD30495</title><shortName>J/ApJ/812/12</shortName><identifier>ivo://CDS.VizieR/J/ApJ/812/12</identifier><altIdentifier>doi:10.26093/cds/vizier.18120012</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Egeland R.</name></creator><creator><name>Metcalfe T.S.</name></creator><creator><name>Hall J.C.</name></creator><creator><name>Henry G.W.</name></creator><date role="Updated">2017-06-20T13:16:11Z</date><date role="Created">2016-02-22T13:07:12Z</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>medium-band-photometry</subject><subject>g-stars</subject><description>A growing body of evidence suggests that multiple dynamo mechanisms can drive magnetic variability on different timescales, not only in the Sun but also in other stars. Many solar activity proxies exhibit a quasi-biennial (~2yr) variation, which is superimposed upon the dominant 11 year cycle. A well-characterized stellar sample suggests at least two different relationships between rotation period and cycle period, with some stars exhibiting long and short cycles simultaneously. Within this sample, the solar cycle periods are typical of a more rapidly rotating star, implying that the Sun might be in a transitional state or that it has an unusual evolutionary history. In this work, we present new and archival observations of dual magnetic cycles in the young solar analog HD 30495, a ~1Gyr old G1.5V star with a rotation period near 11 days. This star falls squarely on the relationships established by the broader stellar sample, with short-period variations at ~1.7yr and a long cycle of ~12yr. We measure three individual long-period cycles and find durations ranging from 9.6 to 15.5yr. We find the short-term variability to be intermittent, but present throughout the majority of the time series, though its occurrence and amplitude are uncorrelated with the longer cycle. These essentially solar-like variations occur in a Sun-like star with more rapid rotation, though surface differential rotation measurements leave open the possibility of a solar equivalence.</description><source format="bibcode">2015ApJ...812...12E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/812/12</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/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/L8">J/A+A/551/L8 : Chromospheric activity of field stars (Pace, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/L26">J/ApJ/763/L26 : SMARTS observations of eps Eridani (Metcalfe+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A8">J/A+A/531/A8 : Activity indexes and velocities for 890 stars (Jenkins+, 2011)</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/A+A/520/A79">J/A+A/520/A79 : FGK stars chromospheric activity (Martinez-Arnaiz+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/312">J/AJ/138/312 : Activity of bright solar analogs (Hall+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/483/903">J/A+A/483/903 : Mount Wilson index for FGK stars (Buccino+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/469/309">J/A+A/469/309 : Chromospheric activity in late-type stars (Cincunegui+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/161">J/AJ/132/161 : NStars project: The southern sample. I. (Gray+, 2006)</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/A+A/365/545">J/A+A/365/545 : Remnant disks around MS stars IR flux (Habing+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/457/L99">J/ApJ/457/L99 : 25yr CaII-HK obs. of F-K nearby stars (Baliunas+, 1996)</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/812/12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/812/12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/812/12</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/812/12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/812/12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/812/12</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></coverage><tableset><schema><name>default</name><table><name>J/ApJ/812/12/table3</name><description>S-index observations of HD 30495</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>HJD</name><description>[39787.4/56965.8] Heliocentric Julian Date; HJD-2400000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>S</name><description>[0.24/0.39] The S-index (1)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_S</name><description>[0.0004/0.04] The 1-sigma uncertainty in S</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Inst</name><description>Instrument used (CPS, HARPS, MWO, SMARTS or SSS)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column></table><table><name>J/ApJ/812/12/table4</name><description>Photometric observations of HD 30495</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>HJD</name><description>[49239.9/57080.7] Heliocentric Julian Date; HJD-2400000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>(P-C1)b</name><description>[-0.5/-0.3] HD30495-HD31414 differential mag in b</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(P-C1)y</name><description>[-0.3/-0.1] HD30495-HD31414 differential mag in y</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(P-C2)b</name><description>[-0.3/-0.1] HD30495-HD30606 differential mag in b</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(P-C2)y</name><description>[-0.3/-0.2] HD30495-HD30606 differential mag in y</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(C2-C1)b</name><description>[-0.2/-0.1] HD30606-HD31414 differential mag in b</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(C2-C1)y</name><description>[0.04/0.08] HD30606-HD31414 differential mag in y</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>