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20122026
most citedPrecise Radial Velocities of Giant Stars VII. Occurrence Rate of Giant Extrasolar Planets as a Function of Mass and Metallicity

252 citations · 3.4k across the 90 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.EP2019★ 18 cited

TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS

Allen B. Davis, Songhu Wang, Matias Jones +46

We report the discovery and confirmation of two new hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS): TOI 564 b and TOI 905 b. The transits of these two…

astro-ph.EP2019★ 17 cited

Radial-velocity jitter of stars as a function of observational timescale and stellar age

Stefan S. Brems, Martin Kürster, Trifon Trifonov +2

Stars show various amounts of radial velocity (RV) jitter due to varying stellar activity levels. The typical amount of RV jitter as a function of stellar age and observational tim…

astro-ph.EP2019★ 56 cited

TOI-677 b: A Warm Jupiter (P=11.2d) on an eccentric orbit transiting a late F-type star

Andrés Jordán, Rafael Brahm, Néstor Espinoza +46

We report the discovery of TOI-677 b, first identified as a candidate in light curves obtained within Sectors 9 and 10 of the Transiting Exoplanet Survey Satellite (TESS) mission a…

astro-ph.EP2019★ 3 cited

Precise radial velocities of giant stars XIII. A second Jupiter orbiting in 4:3 resonance in the 7 CMa system

R. Luque, T. Trifonov, S. Reffert +8

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…

astro-ph.EP2019★ 130 cited

A giant exoplanet orbiting a very low-mass star challenges planet formation models

J. C. Morales, A. J. Mustill, I. Ribas +179

Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreeme…

astro-ph.EP2019★ 155 cited

The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star

M. Zechmeister, S. Dreizler, I. Ribas +182

Context. Teegarden's Star is the brightest and one of the nearest ultra-cool dwarfs in the solar neighbourhood. For its late spectral type (M7.0V), the star shows relatively little…

astro-ph.SR2019★ 4 cited

Variables in the Southern Polar Region Evryscope 2016 Dataset

Jeffrey K. Ratzloff, Henry T. Corbett, Nicholas M. Law +6

The regions around the celestial poles offer the ability to find and characterize long-term variables from ground-based observatories. We used multi-year Evryscope data to search f…

astro-ph.SR2019★ 20 cited

Precise radial velocities of giant stars. XI. Two brown dwarfs in 6:1 mean motion resonance around the K giant star Ophiuchi

Andreas Quirrenbach, Trifon Trifonov, Man Hoi Lee +1

We present radial-velocity (RV) measurements for the K giant Oph (= HIP88048, HD163917, HR6698), which reveal two brown dwarf companions with a period ratio close to 6:1. For o…

astro-ph.SR2019★ 31 cited

Precise radial velocities of giant stars. XII. Evidence against the proposed planet Aldebaran b

Katja Reichert, Sabine Reffert, Stephan Stock +2

Radial-velocity variations of the K giant star Aldebaran ( Tau) were first reported in the early 1990s. After subsequent analyses, the radial-velocity variability with a period…

astro-ph.EP2019★ 37 cited

K2-290: a warm Jupiter and a mini-Neptune in a triple-star system

M. Hjorth, A. B. Justesen, T. Hirano +41

We report the discovery of two transiting planets orbiting K2-290 (EPIC 249624646), a bright (V=11.11) late F-type star residing in a triple-star system. It was observed during Cam…

astro-ph.EP2019★ 22 cited

Two Jovian planets around the giant star HD202696. A growing population of packed massive planetary pairs around massive stars?

Trifon Trifonov, Stephan Stock, Thomas Henning +6

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…