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Table · dataset · 2025

Radial velocities of TOI-1266 from MAROON-X

Listed in IVOA Registry (Virtual Observatory)

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.

Description

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.

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Catalogue records · 2

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/aj/169/10911 d agoJSON v1
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concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0