期刊
ASTRONOMY & ASTROPHYSICS
卷 622, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201731173
关键词
planetary systems; techniques: radial velocities; techniques: spectroscopic; methods: data analysis; stars: general
资金
- Swiss National Science Foundation (SNSF)
- Geneva University
- SNSF
- Society in Science-The Branco Weiss Fellowship
- Fundacao para a Ciencia e a Tecnologia (FCT, Portugal)
- FEDER through COMPETE2020 [UID/FIS/04434/2013 & POCI-01-0145-FEDER-007672, PTDC/FIS-AST/1526/2014 & POCI-01-0145-FEDER-016886]
- FCT [IF/00169/2012/CP0150/CT0002]
- POPH/FSE (EC)
- Fundacao para a Ciencia e a Tecnologia (FCT) [IF/00169/2012/CP0150/CT0002, IF/01037/2013/CP1191/CT0001]
- POPH/FSE (EC) by FEDER through the program Programa Operacional de Factores de Competitividade - COMPETE
- STFC [ST/M001296/1]
- STFC [ST/P000495/1, ST/R000824/1, ST/M001296/1] Funding Source: UKRI
- Fundação para a Ciência e a Tecnologia [IF/00169/2012/CP0150/CT0002, IF/01037/2013/CP1191/CT0001] Funding Source: FCT
Context. We present radial-velocity measurements of eight stars observed with the HARPS Echelle spectrograph mounted on the 3.6-m telescope in La Silla (ESO, Chile). Data span more than ten years and highlight the long-term stability of the instrument. Aims. We search for potential planets orbiting HD20003, HD20781, HD21693, HD31527, HD45184, HD51608, HD134060 and HD136352 to increase the number of known planetary systems and thus better constrain exoplanet statistics. Methods. After a preliminary phase looking for signals using generalized Lomb-Scargle periodograms, we perform a careful analysis of all signals to separate bona-fide planets from signals induced by stellar activity and instrumental systematics. We finally secure the detection of all planets using the efficient MCMC available on the Data and Analysis Center for Exoplanets (DACE web-platform), using model comparison whenever necessary. Results. In total, we report the detection of twenty new super-Earth to Neptune-mass planets, with minimum masses ranging from 2 to 30 M-Earth and periods ranging from 3 to 1300 days, in multiple systems with two to four planets. Adding CORALIE and HARPS measurements of HD20782 to the already published data, we also improve the characterization of the extremely eccentric Jupiter orbiting this visual companion of HD20781.
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