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Related papers: A 4-Planet System Orbiting the K0V Star HD 141399

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The search for exoplanets has revealed a diversity of planetary system architectures, the vast majority of which diverge significantly from the template of the solar system. In particular, giant planets beyond the snow line are relatively…

Earth and Planetary Astrophysics · Physics 2023-10-03 Stephen R. Kane

We report the discovery of a multi-planet system orbiting HD 106315, a rapidly rotating mid F-type star, using data from the K2 mission. HD 106315 hosts a $2.51\pm0.12\,R_\oplus$ sub-Neptune in a 9.5 day orbit, and a…

We report the discovery of a second planet orbiting the K giant star 7 CMa based on 166 high-precision radial velocities obtained with Lick, HARPS, UCLES and SONG. The periodogram analysis reveals two periodic signals of approximately 745…

Earth and Planetary Astrophysics · Physics 2019-11-06 R. Luque , T. Trifonov , S. Reffert , A. Quirrenbach , M. H. Lee , S. Albrecht , M. Fredslund Andersen , V. Antoci , F. Grundahl , C. Schwab , V. Wolthoff

Aims. Our new program with HARPS aims to detect mean motion resonant planetary systems around stars which were previously reported to have a single bona fide planet, often based only on sparse radial velocity data. Methods. Archival and new…

Earth and Planetary Astrophysics · Physics 2017-06-14 T. Trifonov , M. Kürster , M. Zechmeister , O. V. Zakhozhay , S. Reffert , M. H. Lee , F. Rodler , S. S. Vogt , S. S. Brems

(Abreviated) Continued radial velocity monitoring of the nearby M4V red dwarf star GJ~876 with Keck/HIRES has revealed the presence of a Uranus-mass fourth planetary companion in the system. The new planet has a mean period of $P_e=126.6$…

Earth and Planetary Astrophysics · Physics 2015-05-19 Eugenio J. Rivera , Gregory Laughlin , R. Paul Butler , Steven S. Vogt , Nader Haghighipour , Stefano Meschiari

We present evidence for a new two-planet system around the giant star HD202696 (= HIP105056, BD+26 4118). The discovery is based on public HIRES radial velocity measurements taken at Keck Observatory between July 2007 and September 2014. We…

This paper reports on the detection of a planetary system with three Super-Earths orbiting HD40307. HD40307 is a K2V metal-deficient star at a distance of only 13 parsec, part of the HARPS GTO high-precision planet-search programme. The…

Astrophysics · Physics 2009-11-13 M. Mayor , S. Udry , C. Lovis , F. Pepe , D. Queloz , W. Benz , J. -L. Bertaux , F. Bouchy , C. Mordasini , D. Segransan

The Kepler mission has revealed a great diversity of planetary systems and architectures, but most of the planets discovered by Kepler orbit faint stars. Using new data from the K2 mission, we present the discovery of a five planet system…

Multi-planet systems exhibit a diversity of architectures that diverge from the solar system and contribute to the topic of exoplanet demographics. Radial velocity (RV) surveys form a crucial component of exoplanet surveys, as their long…

We report the characterisation of a multi-planetary system composed of five exoplanets orbiting the K-dwarf HD~23472 (TOI-174). In addition to the two super-Earths that were previously confirmed, we confirm and characterise three Earth-size…

Earth and Planetary Astrophysics · Physics 2022-09-28 S. C. C. Barros , O. D. S. Demangeon , Y. Alibert , A. Leleu , V. Adibekyan , C. Lovis , D. Bossini , S. G. Sousa , N. Hara , the ESPRESSO team

We report the detection of a large mass planet orbiting around the K0 metal-rich subgiant HD38801 ($V=8.26$) by precise radial velocity (RV) measurements from the Subaru Telescope and the Keck Telescope. The star has a mass of…

For the past 3 years we have been monitoring 62 K giant stars using precise stellar radial velocity (RV) measurements with the 2m Alfred Jensch telescope of the Th\"uringer Landessternwarte Tautenburg (TLS). To probe the dependence of…

Earth and Planetary Astrophysics · Physics 2015-05-13 M. P. Doellinger , A. P. Hatzes , L. Pasquini , E. W. Guenther , M. Hartmann , L. Girardi

We report precise Doppler measurements of seven subgiants from Keck Observatory. All seven stars show variability in their radial velocities consistent with planet-mass companions in Keplerian orbits. The host stars have masses ranging from…

Doppler observations from Keck Observatory have revealed a triple planet system orbiting the nearby mid-type K dwarf, HIP 57274. The inner planet, HIP 57274b, is a super-Earth with \msini\ = 11.6 \mearth (0.036 \mjup), an orbital period of…

Based on two decades of radial velocity (RV) observations using Keck/HIRES and McDonald/Tull, and more recent observations using the Automated Planet Finder, we found that the nearby star HR 5183 (HD 120066) hosts a 3$M_J$ minimum mass…

We re-analyze the precision radial velocity (RV) data of HD188015, HD114729, HD190360, HD147513 and HD208487. All these stars are supposed to host Jovian companions in long-period orbits. We test a hypothesis that the residuals of the…

Astrophysics · Physics 2007-05-23 Krzysztof Gozdziewski , Cezary Migaszewski

We analyze 8 years of precise radial velocity measurements from the Keck Planet Search, characterizing the detection threshold, selection effects, and completeness of the survey. We carry out a systematic search for planets by assessing the…

We present the detection of three super-Earths transiting the cool star LP415-17, monitored by K2 mission in its 13th campaign. High resolution spectra obtained with HARPS-N/TNG showed that the star is a mid-late K dwarf. Using spectral…

We have enlarged the sample of stars in the planet search at Lick Observatory. Doppler measurements of 82 new stars observed at Lick Observatory, with additional velocities from Keck Observatory, have revealed two new planet candidates. The…

Astrophysics · Physics 2016-08-30 D. A. Fischer , G. W. Marcy , R. P. Butler , S. S. Vogt , K. Apps

We report the discovery of a compact multi-planet system orbiting the relatively nearby (78pc) and bright ($K=8.9$) K-star, K2-266 (EPIC248435473). We identify up to six possible planets orbiting K2-266 with estimated periods of P$_b$ =…