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<ri:Resource created="2025-10-06T09:38:30Z" status="active" updated="2026-07-02T12:00:07Z" 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>Gaia-Chandra members of 7-25Myr clusters with ZTF</title><shortName>J/ApJ/952/63</shortName><identifier>ivo://CDS.VizieR/J/ApJ/952/63</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xr-1z</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Getman K.V.</name></creator><creator><name>Feigelson E.D.</name></creator><creator><name>Garmire G.P.</name></creator><date role="Updated">2026-07-02T12:00:07Z</date><date role="Created">2025-10-06T09:38:30Z</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>g-stars</subject><subject>pre-main-sequence-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>x-ray-sources</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>effective-temperature</subject><description>We study the four-dimensional relationships between magnetic activity, rotation, mass, and age for solar-type stars in the age range 5-25Myr. This is the late-pre-main-sequence (l-PMS) evolutionary phase when rapid changes in a star's interior may lead to changes in the magnetic dynamo mechanisms. We carefully derive rotational periods and spot sizes for 471 members of several l-PMS open clusters using photometric light curves from the Zwicky Transient Facility. Magnetic activity was measured in our previous Chandra-based study, and additional rotational data were obtained from other work. Several results emerge. Mass-dependent evolution of rotation through the l-PMS phase agrees with astrophysical models of stellar angular momentum changes, although the data suggest a subpopulation of stars with slower initial rotations than commonly assumed. There is a hint of the onset of unsaturated tachoclinal dependency of X-ray activity on rotation, as reported by Argiroffi+ (2016, J/A+A/589/A113), but this result is not confidently confirmed. Both X-ray luminosity and starspot area decrease approximately as t^-1^ for solar-mass stars, suggesting that spot magnetic fields are roughly constant and l-PMS stars follow the universal solar-scaling law between the X-ray luminosity and surface magnetic flux. Assuming convective dynamos are dominant, theoretical magnetic fluxes fail to reveal the universal law for l-PMS stars that enter late Henyey tracks. Altogether we emerge with a few lines of evidence suggesting that the transition from the turbulent to solar-type dynamo occurs at the later stages of l-PMS evolution as stars approach the zero-age main sequence.</description><source format="bibcode">2023ApJ...952...63G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/952/63</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/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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Total number of cluster members identified across entire Chandra fields</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Nmcent</name><description>[90/1291]? Stellar members located in the central parts of the clusters</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Nztf</name><description>Number of members with ZTF data (link to Table 1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Nadd</name><description>Number of additional members with previously published rotation periods (link to Table 3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Dist</name><description>[319/2552]? Median cluster distance from the Sun</description><unit>pc</unit><ucd>pos.distance;stat.median;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Dist</name><description>[1/34]? 68% bootstrap error on Dist</description><unit>pc</unit><ucd>stat.error;pos.distance;stat.median</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Av</name><description>[0.2/2.1]? Cluster average extinction in visual band</description><unit>mag</unit><ucd>phys.absorption;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age</name><description>[7/25]? Cluster age</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Mlim</name><description>[0.4/1]? Mass completeness limits for our cluster member samples</description><unit>solMass</unit><ucd>phys.mass;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/952/63/table1</name><description>5-25Myr PMS stars with rotation and X-ray properties</description><column><name>Cluster</name><description>Cluster identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><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>Seq</name><description>[1/566] Sequential source number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[34.4/110] Gaia DR3 Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-25.1/62.6] Gaia DR3 Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>logTeff</name><description>[3.48/4.3] Log effective temperature (1)</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.27/6.5] Mass (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLbol</name><description>[-1.5/3.2] Log bolometric luminosity (1)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PRot</name><description>[0.2/32.51] Rotation period (2)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Amp</name><description>[0.002/0.4] Peak-to-peak photometric amplitude (3)</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLx</name><description>[28.7/31.5]? Log Chandra 0.5-8keV X-ray luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLxup</name><description>[28.47/30.4]? Upper log Chandra 0.5-8keV X-ray luminosity limit; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tau</name><description>[6.2/403.7]? Convective turnover timescale (4)</description><unit>d</unit><ucd>time.scale</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PapI</name><description>Display data from Paper I (Getman+ 2022, J/ApJ/935/43)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/952/63/table3</name><description>*Gaia-DR3 masses for stars with previously published rotation periods</description><column><name>Cluster</name><description>Cluster identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>B-R</name><description>[-0.05/4.8] Gaia DR3 (Blue-Red) passband color</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_B-R</name><description>[0.005/0.1] Uncertainty in B-R</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logTeff</name><description>[3.4/4.24] Log effective temperature (1)</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.06/5] Mass (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLbol</name><description>[-2.54/2.8] Log Bolometric luminosity (1)</description><unit>log(solLum)</unit><ucd>phys.luminosity;phot.flux.bol</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PRot</name><description>[0.04/27.1] Rotation period (2)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Amp</name><description>[0.002/0.6]? Peak-to-peak photometric amplitude (3)</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gaia</name><description>Display data from Gaia DR3 (I/355) within 1.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><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>RAJ2000</name><description>[34.48/259] Gaia DR3 Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-72.7/57.3] Gaia DR3 Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Gmag</name><description>[5.8/20.1] Gaia DR3 G band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gmag</name><description>[0.003/0.03] Uncertainty in Gmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/952/63/table4</name><description>New HRD statuses for l-PMS stars from Paper I (Getman+ 2022, J/ApJ/935/43)</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>Cluster</name><description>Cluster identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>RAJ2000</name><description>[34.4/194] Gaia DR3 Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-61.8/62.6] Gaia DR3 Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>phHRD</name><description>[1/13.54] Updated stellar evolutionary phase (1)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PapI</name><description>Display data from Paper I (Getman+ 2022, J/ApJ/935/43)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>