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<ri:Resource created="2025-12-04T14:29:22Z" status="active" updated="2026-07-02T11:45:17Z" 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>Radial velocities of TOI-1266 from MAROON-X</title><shortName>J/AJ/169/109</shortName><identifier>ivo://CDS.VizieR/J/AJ/169/109</identifier><altIdentifier>doi:10.26093/cds/vizier/be-59-3d</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tyler D.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Rogers J.</name></creator><creator><name>Lubin J.</name></creator><creator><name>Seifhart A.</name></creator><creator><name>Bean J.L.,Brady M.</name></creator><creator><name>Luque R.</name></creator><date role="Updated">2026-07-02T11:45:17Z</date><date role="Created">2025-12-04T14:29:22Z</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>radial-velocity</subject><subject>m-stars</subject><subject>dwarf-stars</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>We present an analysis of 126 new radial velocity measurements from the MAROON-X spectrograph to investigate the TOI-1266 system, which hosts two known transiting sub-Neptunes at 10.8 and 18.8 days. We integrated our measurements with existing HARPS-N measurements for this system and derived revised masses for TOI-1266 b and c of M_b_=4.09+/-0.45M_{Earth}_ and M_c_=2.64+/-0.52M_{Earth}_, respectively. The Keplerian fit from the combined datasets enabled an ~35% and ~41% improvement in mass precision for planet b and c, respectively, compared to the previously published values. With bulk densities of {rho}_b_=1.25+/-0.21g/cm3 and {rho}_c_=1.51+/-0.39g/cm, the planets are among the lowest density sub-Neptunes orbiting an M dwarf. They are both consistent with rocky cores surrounded by hydrogen helium envelopes. TOI-1266 c may also be consistent with a water-rich composition, but we disfavor that interpretation from an Occam's razor perspective.</description><source format="bibcode">2025AJ....169..109T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/169/109</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/MNRAS/422/2024">J/MNRAS/422/2024 : X-ray-age relation &amp; exoplanet evaporation (Jackson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/45">J/ApJ/807/45 : Potentially habitable planets orbit. M dwarfs (Dressing+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/109">J/AJ/154/109 : California-Kepler Surv. (CKS). III. 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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>[2459660/2460140] Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-7.32/7.52] 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>[0.64/2.8] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Arm</name><description>Spectrograph arm identifier (1)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>