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<ri:Resource created="2026-04-17T14:01:17Z" status="active" updated="2026-08-03T07:20:11Z" 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>TESS &amp; KPF: TOI-2364 light &amp; radial velocity curves</title><shortName>J/AJ/170/34</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/34</identifier><altIdentifier>doi:10.26093/cds/vizier/be-5a-12</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tamburo P.</name></creator><creator><name>Yee S.W.</name></creator><creator><name>Garcia-mejia J.</name></creator><creator><name>Stefansson G.</name></creator><creator><name>Charbonneau D.,Bieryla A.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Fulton B.J.</name></creator><creator><name>Householder A.</name></creator><date role="Updated">2026-08-03T07:20:11Z</date><date role="Created">2026-04-17T14:01:17Z</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>infrared-photometry</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>We measure the true obliquity of TOI-2364, a K dwarf with a sub-Saturn-mass (M_p_=0.18M_J_) transiting planet on the upper edge of the hot-Neptune desert. We used new Rossiter-McLaughlin observations gathered with the Keck Planet Finder to measure the sky-projected obliquity {lambda}=7{deg}+10{deg}-11{deg}. Combined with a stellar rotation period of 23.47+/-0.29days measured with photometry from the Tierras Observatory, this yields a stellar inclination of 90{deg}+/-13{deg} and a true obliquity {psi}=15:6+7:7-7:3, indicating that the planet's orbit is well aligned with the rotation axis of its host star. The determination of {psi} is important for investigating a potential bimodality in the orbits of short-period sub-Saturns around cool stars, which tend to be either aligned with or perpendicular to their host stars' spin axes.</description><source format="bibcode">2025AJ....170...34T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/34</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/PASP/134/H2001">J/PASP/134/H2001 : Stellar obliquities in exoplanetary syst. (Albrecht+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/474/2094">J/MNRAS/474/2094 : Inferring probabilistic stellar rot. periods (Angus+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/168/185">J/AJ/168/185 : HATS-38b &amp; WASP-139b: LCs &amp; RVs (Espinoza-Retamal+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/690/A379">J/A+A/690/A379 : Obliquities of exoplanet host stars (Knudstrup+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/510/5623">J/MNRAS/510/5623 : Study of Kepler's FGKM stars (Masuda+, 2022)</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/557/L10">J/A+A/557/L10 : Rotation periods of 12000 Kepler stars (Nielsen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/635/A43">J/A+A/635/A43 : Stellar rot. periods from K2 Campaigns 0-18 (Reinhold+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/931/L15">J/ApJ/931/L15 : Obs. of two transits of GJ 3470b with NEID (Stefansson+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/253">J/AJ/163/253 : The Perkins INfrared Exosatellite Survey. 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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>Sector</name><description>TESS sector identifier (1)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>BJD</name><description>[2458471/2460687] Barycentric Julian Date; TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NFlux</name><description>[0.98/1.01] Normalized flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_NFlux</name><description>[6e-4/3e-3] Uncertainty in NFlux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/AJ/170/34/fig3b</name><description>KeplerCam light curve of TOI-2364</description><column><name>NFlux</name><description>[0.98/1.02] Normalized flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_NFlux</name><description>[1.1e-3/1.2e-3] Uncertainty in NFlux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Air</name><description>[-0.3/1] Airmass</description><ucd>obs.airMass</ucd><dataType xsi:type="vs:VOTableType">double</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>BJD</name><description>[2460239/2460241] Barycentric Julian Date; TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/AJ/170/34/fig3c</name><description>Kepler Planet Finder radial velocity curve of TOI-2364</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>BJD</name><description>[2460239/2460241] Barycentric Julian Date; TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[54.7/54.8] Radial velocity</description><unit>m/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[1.8e-3/2.2e-3] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>