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<ri:Resource created="2022-09-09T15:12:44Z" 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>Planets Across Space and Time (PAST). I.</title><shortName>J/ApJ/909/115</shortName><identifier>ivo://CDS.VizieR/J/ApJ/909/115</identifier><altIdentifier>doi:10.26093/cds/vizier.19090115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen D.-C.</name></creator><creator><name>Xie J.-W.</name></creator><creator><name>Zhou J.-L.</name></creator><creator><name>Dong S.</name></creator><creator><name>Liu C.</name></creator><creator><name>Wang H.-F.</name></creator><creator><name>Xiang M.-S.,Huang Y.</name></creator><creator><name>Luo A.</name></creator><creator><name>Zheng Z.</name></creator><date role="Updated">2024-11-06T20:23:13Z</date><date role="Created">2022-09-09T15:12:44Z</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>exoplanets</subject><subject>stellar-ages</subject><subject>proper-motions</subject><subject>radial-velocity</subject><subject>metallicity</subject><subject>surveys</subject><subject>visible-astronomy</subject><description>Over 4000 exoplanets have been identified and thousands of candidates are to be confirmed. The relations between the characteristics of these planetary systems and the kinematics, Galactic components, and ages of their host stars have yet to be well explored. To address these questions, we conduct a research project, dubbed Planets Across Space and Time (PAST). To do this, one of the key steps is to accurately characterize the planet host stars. In this paper, Paper I of the PAST series, we revisit the kinematic method for classification of Galactic components and extend the applicable range of velocity ellipsoid from ~100pc to ~1500pc from the Sun in order to cover most known planet hosts. Furthermore, we revisit the age-velocity dispersion relation (AVR), which allows us to derive kinematic ages with a typical uncertainty of 10-20% for an ensemble of stars. Applying the above revised methods, we present a catalog of kinematic properties (i.e., Galactic positions, velocities, and the relative membership probabilities among the thin disk, thick disk, Hercules stream, and the halo) as well as other basic stellar parameters for 2174 host stars of 2872 planets by combining data from Gaia, LAMOST, APOGEE, RAVE, and the NASA exoplanet archive. The revised kinematic method and AVR, as well as the stellar catalog of kinematic properties and ages, lay the foundation for future studies of exoplanets in space and time in the Galactic context.</description><source format="bibcode">2021ApJ...909..115C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/909/115</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/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/279">III/279 : RAVE 5th data release (Kunder+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/153">V/153 : LAMOST DR4 catalogs (Luo+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>r_Teff</name><description>[1/5] Source for Teff (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[-1.16/5.63]? Surface gravity, log</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_logg</name><description>[1/5] Source for logg (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Fe/H]</name><description>[-2.15/0.7]? Metallicity</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_[Fe/H]</name><description>[0/5]? Source for [Fe/H]</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>aFe</name><description>[-0.33/0.8]? {alpha} elements abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_aFe</name><description>[0/4]? Source for aFe (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RV</name><description>[-122/245] Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R</name><description>[6.9/11.7] Galactocentric Cylindrical radial distance</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Theta</name><description>[-2.2/4.2] Galactocentric Cylindrical azimuth angle, {theta}</description><unit>deg</unit><ucd>instr.offset</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>[-0.87/1.01] Galactocentric Cylindrical vertical height</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VR</name><description>[-149/163] Galactocentric Cylindrical R velocities</description><unit>km/s</unit><ucd>phys.veloc;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>VT</name><description>[-40/336] Galactocentric Cylindrical {theta} velocities</description><unit>km/s</unit><ucd>phys.veloc;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>VZ</name><description>[-96/89] Galactocentric Cylindrical Z velocities</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ULSR</name><description>[-140/181] Cartesian Galactocentric X velocity to the LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_ULSR</name><description>[0.003/68] Uncertainty in ULSR</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VLSR</name><description>[-278/97] Cartesian Galactocentric Y velocity to the LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_VLSR</name><description>[0.0009/76] Uncertainty in VLSR</description><unit>km/s</unit><ucd>stat.error;phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WLSR</name><description>[-89/89] Cartesian Galactocentric Z velocity to the LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_WLSR</name><description>[0.0013/75] Uncertainty in WLSR</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TD/D</name><description>[0.007/8.9e+23] Thick disc to thin disc membership probability ratio</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TD/H</name><description>[1e-5/25550] Thick disc to halo membership probability ratio</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Her/D</name><description>[3.6e-109/17] Hercules stream to thin disc membership probability ratio</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Her/TD</name><description>[4e-133/13] Hercules stream to thick disk membership probability ratio</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>APOGEE</name><description>APOGEE unique spectral ID (2MHHMMSSss+DDMMSSs; J2000)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>RAVE</name><description>RAVE unique spectral ID (JHHMMSS.s+DDMMSS)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>HName</name><description>NASA Exoplanet archive unique planet host name</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</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=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</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>Gaia</name><description>Unique Gaia DR2 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>LAMOST</name><description>LAMOST unique spectral ID</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="36*">char</dataType></column><column><name>KIC</name><description>[757450/12885212]? Kepler Input Catalog ID</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RA_ICRS</name><description>Gaia DR2 Barycentric Right Ascension (ICRS) at epoch 2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column></table></schema></tableset></ri:Resource>