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Table · dataset · 2026

HD 125136, HD 127195, and HD 220218 RV curves

Listed in IVOA Registry (Virtual Observatory)

We extend the planetary census around massive stellar hosts through a long-term campaign of high-precision radial velocity (RV) measurements on evolved stars.

Description

We analyse data acquired with the CORALIE spectrograph covering 15-18 years on HD 125136, HD 127195, and HD 220218. Stellar parameters are derived through different methods for a comprehensive characterization of each star.

We then evaluate the presence of planetary signals in the RV time series using the Bayesian inference tool kima. Finally, we design an observing strategy aimed at mitigating the impact of pulsations on evolved stars and test its effectiveness on the low-luminosity red giant HD 127195. We detect signals that are accurately modelled by Keplerian curves in the RV data of the three stars: one on HD 125136, two on HD 127195, and one on HD 220218.

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While the signals on the first two stars seem to be of planetary origin, the signal on the third one shows several signs of stellar activity. We therefore identify a planetary companion around HD 125136 with a minimum mass of 2.26M_Jup_ on an 850d orbit, and on HD 127195 we identify a system composed of planets with 0.66M_Jup_ and 0.78 MJup with orbital periods of 535d and 834d, respectively. We detect three massive planets around two low-luminosity red giant stars in a region of the parameter space that is poorly populated in both stellar mass and planetary orbital periods.

The dedicated observing campaign on HD 127195 showcases how stellar pulsations can be efficiently averaged out to below 5m/s in low-luminosity giant stars.

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Provenance · 1 source records, 9 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/712/a14312 d agoJSON v1
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