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<ri:Resource created="2024-04-22T07:49:49Z" 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>54 years S-index measurements for {lambda} Ser</title><shortName>J/AJ/166/167</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/167</identifier><altIdentifier>doi:10.26093/cds/vizier.51660167</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Metcalfe T.S.</name></creator><creator><name>Buzasi D.</name></creator><creator><name>Huber D.</name></creator><creator><name>Pinsonneault M.H.</name></creator><creator><name>van Saders J.L.,Ayres T.R.</name></creator><creator><name>Basu S.</name></creator><creator><name>Drake J.J.</name></creator><creator><name>Egeland R.</name></creator><creator><name>Kochukhov O.</name></creator><creator><name>Petit P.,Saar S.H.</name></creator><creator><name>See V.</name></creator><creator><name>Stassun K.G.</name></creator><creator><name>Li Y.</name></creator><creator><name>Bedding T.R.</name></creator><creator><name>Breton S.N.,Finley A.J.</name></creator><creator><name>Garcia R.A.</name></creator><creator><name>Kjeldsen H.</name></creator><creator><name>Nielsen M.B.</name></creator><creator><name>Ong J.M.J.,Rorsted J.L.</name></creator><creator><name>Stokholm A.</name></creator><creator><name>Winther M.L.</name></creator><creator><name>Clark C.A.</name></creator><creator><name>Godoy-Rivera D.,Ilyin I.V.</name></creator><creator><name>Strassmeier K.G.</name></creator><creator><name>Jeffers S.V.</name></creator><creator><name>Marsden S.C.</name></creator><creator><name>Vidotto A.A.,Baliunas S.</name></creator><creator><name>Soon W.</name></creator><date role="Updated">2024-11-06T20:17:59Z</date><date role="Created">2024-04-22T07:49:49Z</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><description>The bright star {lambda}Ser hosts a hot Neptune with a minimum mass of 13.6M{Earth} and a 15.5day orbit. It also appears to be a solar analog, with a mean rotation period of 25.8days and surface differential rotation very similar to the Sun. We aim to characterize the fundamental properties of this system and constrain the evolutionary pathway that led to its present configuration. We detect solar-like oscillations in time series photometry from the Transiting Exoplanet Survey Satellite, and we derive precise asteroseismic properties from detailed modeling. We obtain new spectropolarimetric data, and we use them to reconstruct the large-scale magnetic field morphology. We reanalyze the complete time series of chromospheric activity measurements from the Mount Wilson Observatory, and we present new X-ray and ultraviolet observations from the Chandra and Hubble space telescopes. Finally, we use the updated observational constraints to assess the rotational history of the star and estimate the wind braking torque. We conclude that the remaining uncertainty on the stellar age currently prevents an unambiguous interpretation of the properties of {lambda}Ser, and that the rate of angular momentum loss appears to be higher than for other stars with a similar Rossby number. Future asteroseismic observations may help to improve the precision of the stellar age.</description><source format="bibcode">2023AJ....166..167M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/167</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/ApJ/457/L99">J/ApJ/457/L99 : 25yr CaII-HK obs of F-K nearby stars (Baliunas+, 1996)</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/other/A+ARV/18.67">J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/3517">J/MNRAS/444/3517 : BCool survey of solar-type stars (Marsden+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A23">J/A+A/580/A23 : Stroemgren-Crawford uvby{beta} photometry (Paunzen, 2015)</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/AJ/152/180">J/AJ/152/180 : Bolometric fluxes of eclipsing bin Tycho-2 (Stassun+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/172">J/ApJ/835/172 : Kepler asteroseismic LEGACY sample. 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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>JD</name><description>[-807/12440] Julian Date ; JD-2440000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SIndex</name><description>[0.13/0.67] S-Index value</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>