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<ri:Resource created="2024-07-01T08:58:05Z" 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>TESS/HIRES radial velocity follow up of TOI-1824</title><shortName>J/AJ/167/282</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/282</identifier><altIdentifier>doi:10.26093/cds/vizier.51670282</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lange S.</name></creator><creator><name>Murphy J.M.A.</name></creator><creator><name>Batalha N.M.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Dressing C.D.,Fulton B.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Huber D.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Kane S.R.</name></creator><creator><name>Petigura E.A.,Robertson P.</name></creator><creator><name>Weiss L.M.</name></creator><creator><name>Behmard A.</name></creator><creator><name>Beard C.</name></creator><creator><name>Blunt S.</name></creator><creator><name>Brinkman C.L.,Chontos A.</name></creator><creator><name>Dai F.</name></creator><creator><name>Dalba P.A.</name></creator><creator><name>Fetherolf T.</name></creator><creator><name>Giacalone S.</name></creator><creator><name>Hill M.L.,Holcomb R.</name></creator><creator><name>Lubin J.</name></creator><creator><name>MacDougall M.G.</name></creator><creator><name>Mayo A.W.</name></creator><creator><name>Mocnik T.,Pidhorodetska D.</name></creator><creator><name>Polanski A.S.</name></creator><creator><name>Rice M.</name></creator><creator><name>Rosenthal L.J.</name></creator><creator><name>Rubenzahl R.A.,Scarsdale N.</name></creator><creator><name>Turtelboom E.V.</name></creator><creator><name>Van Zandt J.</name></creator><creator><name>Ciardi D.R.</name></creator><creator><name>Boyle A.W.</name></creator><date role="Updated">2025-05-05T20:07:57Z</date><date role="Created">2024-07-01T08:58:05Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>We confirm a massive sub-Neptune-sized planet on a P=22.8 days orbit around the star TOI-1824 (Teff=5200 K, V=9.7 mag). TESS first identified TOI-1824 b (formerly TOI-1824.01) as an object of interest in 2020 April after two transits in Sector 22 were matched with a single transit in Sector 21. TOI-1824 was subsequently targeted for ground-based Doppler monitoring with Keck-HIRES and APF-Levy. Using a joint model of the TESS photometry, radial velocities, and Ca ii H and K emission measurements as an activity indicator, we find that TOI-1824b is an unusually dense sub-Neptune. The planet has a radius Rp=2.63{+/-}0.15R{Earth} and mass Mp=18.5{+/-}3.2M{Earth}, implying a bulk density of 5.6{+/-}1.4g/cm^3^. TOI-1824 b's mass and radius situate it near a small group of "superdense sub-Neptunes" (Rp&lt;~3R{Earth} and Mp&gt;~20M{Earth}). While the formation mechanism of superdense sub-Neptunes is a mystery, one possible explanation is the constructive collision of primordial icy cores; such giant impacts would drive atmospheric escape and could help explain these planets' apparent lack of massive envelopes. We discuss TOI-1824b in the context of these overdense planets, whose unique location in the exoplanet mass-radius plane make them a potentially valuable tracer of planet formation.</description><source format="bibcode">2024AJ....167..282L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/282</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/III/150">III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</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/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. 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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>BJD</name><description>[2458967/2459978] Barycentric Julian Date at TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-26.12/30.35] Radial velocity, m/s (1)</description><unit>m.s**-1</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[1.12/6.78] Uncertainty in RVel (2)</description><unit>m.s**-1</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>[0.33/0.406]? Mt. Wilson CaII HK activity index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_SHK</name><description>[0.002/0.002]? 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