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<ri:Resource created="2022-12-19T07:40:54Z" status="active" updated="2025-05-19T09:50:00Z" 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>Candidate members of Cep-Her, RSG-5 and CH-2</title><shortName>J/AJ/164/215</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/215</identifier><altIdentifier>doi:10.26093/cds/vizier.51640215</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bouma L.G.</name></creator><creator><name>Kerr R.</name></creator><creator><name>Curtis J.L.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Hillenbrand L.A.,Howard A.W.</name></creator><creator><name>Kraus A.L.</name></creator><creator><name>Bieryla A.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Huber D.</name></creator><date role="Updated">2023-01-23T14:38:26Z</date><date role="Created">2022-12-19T07:40:54Z</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>open-star-clusters</subject><subject>astrometry</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>Stellar positions and velocities from Gaia are yielding a new view of open cluster dispersal. Here we present an analysis of a group of stars spanning Cepheus (l=100{deg}) to Hercules (l=40{deg}), hereafter the Cep-Her complex. The group includes four Kepler objects of interest: Kepler-1643b (Rp=2.32{+/-}0.13R{Earth}, P=5.3days), KOI-7368b (Rp=2.22{+/-}0.12R{Earth}, P=6.8days), KOI-7913Ab (Rp=2.34{+/-}0.18R{Earth}, P=24.2days), and Kepler-1627 Ab (Rp=3.85{+/-}0.11R{Earth}, P=7.2days). The latter Neptune-sized planet is in part of the Cep-Her complex called the {delta}Lyr cluster. Here we focus on the former three systems, which are in other regions of the association. Based on kinematic evidence from Gaia, stellar rotation periods from TESS, and spectroscopy, these three objects are also ~40 million years (Myr) old. More specifically, we find that Kepler-1643 is 46_-7_^+9^Myr old, based on its membership in a dense subcluster of the complex called RSG-5. KOI-7368 and KOI-7913 are 36_-8_^+10^Myr old, and are in a diffuse region that we call CH-2. Based on the transit shapes and high-resolution imaging, all three objects are most likely planets, with false-positive probabilities of 6x10^-9^, 4x10^-3^, and 1x10^-4^ for Kepler-1643, KOI-7368, and KOI-7913, respectively. These planets demonstrate that mini-Neptunes with sizes of ~2 Earth radii exist at ages of 40Myr.</description><source format="bibcode">2022AJ....164..215B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/164/215</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/J/AJ/106/1059">J/AJ/106/1059 : Lithium in the Pleiades (Soderblom+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/862">J/A+A/372/862 : Lithium abundances in IC 2602 and IC 2391 (Randich+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/1137">J/A+A/439/1137 : PHOENIX model chromospheres of M dwarfs (Fuhrmeister+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/486.375">J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/146">J/AJ/147/146 : Spectroscopy of Tuc-Hor candidate members (Kraus+, 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/ApJ/804/146">J/ApJ/804/146 : Atmospheric parameters for nearby B-F stars (David+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/8">J/AJ/152/8 : Impact of stellar mult. on planetary systems I. 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The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2016.5 (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>vb</name><description>[-10.73/3.24] Latitudinal galactic velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>weight</name><description>[0.02/0.54] Strength of connectivity to other candidate cluster members</description><ucd>stat.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vl*</name><description>[-8.15/8.93] Longitudinal galactic velocity, v_l*_cos(b)</description><unit>km/s</unit><ucd>phys.veloc;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>[-8092/-7983] Galactocentric X position coordinate</description><unit>pc</unit><ucd>pos.cartesian.x;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>[245/373] Galactocentric Y position coordinate</description><unit>pc</unit><ucd>pos.cartesian.y;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>[53/143] Galactocentric Z position coordinate</description><unit>pc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Offset</name><description>[0.003/0.92] Separation between KIC and Gaia DR2 positions</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dmag</name><description>[-0.05/0.04] G-band difference between EDR3 and DR2 source match</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/164/215/table3</name><description>Rotation periods and kinematics for candidate RSG-5 and CH-2 members</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2016.5 (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2016.5 (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></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>EDR3</name><description>Gaia EDR3 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>RAICRS</name><description>[284/306] Gaia EDR3 Right Ascension (ICRS at Epoch=2016.5)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEICRS</name><description>[41/53] Gaia EDR3 Declination (ICRS at Epoch=2016.5)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>plx</name><description>[2.8/4.03] Gaia EDR3 parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RUWE</name><description>[0.74/3.37] Gaia EDR3 renormalized unit weight error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>weight</name><description>[0.001/0.74] Strength of connectivity to other candidate cluster members</description><ucd>stat.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vl*</name><description>[2.09/6] Longitudinal galactic velocity, v_l_cos(b)</description><unit>km/s</unit><ucd>phys.veloc;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vb</name><description>[-3.98/-1.64] Latitudinal galactic velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>[-8101/-8047] Galactocentric X position coordinate</description><unit>pc</unit><ucd>pos.cartesian.x;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>[231/350] Galactocentric Y position coordinate</description><unit>pc</unit><ucd>pos.cartesian.y;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>[40/105] Galactocentric Z position coordinate</description><unit>pc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BP-RP</name><description>[-0.43/3.49] Gaia BP-RP color, minus E(BP-RP)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GMAG</name><description>[-0.68/12.96] Absolute G-band magnitude, corrected for extinction</description><unit>mag</unit><ucd>phys.magAbs;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Cluster</name><description>Cluster, RSG-5 or CH-2</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Prot-A</name><description>[0.61/29.5]? Adopted rotation period if available</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Prot-T</name><description>[0.61/13.4]? TESS rotation period if available</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Prot-Z</name><description>[0.69/29.5]? ZTF rotation period if available</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Confused</name><description>[0/1] Boolean flag; 1=stars are photometrically blended</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>