activity
20172025
most citedThe CARMENES search for exoplanets around M dwarfs -- Planet occurrence rates from a subsample of 71 stars

158 citations · 698 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2025★ 7 cited

The CARMENES search for exoplanets around M dwarfs. Occurrence rates of Earth-like planets around very low-mass stars

A. Kaminski, S. Sabotta, J. Kemmer +24

Aims: Previous estimates of planet occurrence rates in the CARMENES survey indicated increased numbers of planets on short orbits for M dwarfs with masses below 0.34\,M. He…

astro-ph.EP2023★ 6 cited

The CARMENES search for exoplanets around M dwarfs. A sub-Neptunian mass planet in the habitable zone of HN Lib

E. González-Álvarez, J. Kemmer, P. Chaturvedi +29

We report the discovery of HN Lib b, a sub-Neptunian mass planet orbiting the nearby ( = 6.25 pc) M4.0 V star HN Lib detected by our CARMENES radial-velocity (RV) survey…

astro-ph.EP2023★ 22 cited

Gaussian processes for radial velocity modeling Better rotation periods and planetary parameters with the quasi-periodic kernel and constrained priors

Stephan Stock, Jonas Kemmer, Diana Kossakowski +3

In this study we present an analysis of the performance and properties of the quasi-periodic (QP) GP kernel, which is the multiplication of the squared-exponential kernel by the ex…

astro-ph.EP2023★ 96 cited

The CARMENES search for exoplanets around M dwarfs. Guaranteed time observations Data Release 1 (2016-2020)

I. Ribas, A. Reiners, M. Zechmeister +102

The CARMENES instrument was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of n…

astro-ph.EP2023★ 32 cited

The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star

D. Kossakowski, M. Kürster, T. Trifonov +47

We present the discovery of an Earth-mass planet () on a 15.6d orbit of a relatively nearby (9.6pc) and low-mass () M…

astro-ph.EP2022★ 23 cited

A Radial Velocity Study of the Planetary System of Pi Mensae: Improved Planet Parameters for PI Mensae c and a Third Planet on a 125-d Orbit

Artie P. Hatzes, Davide Gandolfi, Judith Korth +33

Pi Men hosts a transiting planet detected by the TESS space mission and an outer planet in a 5.7-yr orbit discovered by RV surveys. We studied this system using new radial velocity…

astro-ph.EP2021★ 158 cited

The CARMENES search for exoplanets around M dwarfs -- Planet occurrence rates from a subsample of 71 stars

S. Sabotta, M. Schlecker, P. Chaturvedi +25

The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 nearby M dwarfs over the past five years as part of its guaranteed time observations (GTO) pr…

astro-ph.EP2021★ 16 cited

TOI-220 : a warm sub-Neptune discovered by TESS

S. Hoyer, D. Gandolfi, D. J. Armstrong +77

In this paper we report the discovery of TOI-220 , a new sub-Neptune detected by the Transiting Exoplanet Survey Satellite (TESS) and confirmed by radial velocity follow-up obse…

astro-ph.EP2020★ 45 cited

Mass determinations of the three mini-Neptunes transiting TOI-125

L. D. Nielsen, D. Gandolfi, D. J. Armstrong +77

The Transiting Exoplanet Survey Satellite, TESS, is currently carrying out an all-sky search for small planets transiting bright stars. In the first year of the TESS survey, steady…

astro-ph.IM2020★ 29 cited

Ondr}ejov echelle spectrograph, ground based support facility for exoplanet missions

Petr Kabath, Marek Skarka, Silvia Sabotta +18

Fulfilling the goals of space-based exoplanetary transit surveys, like Kepler and TESS, is impossible without ground-based spectroscopic follow-up. In particular, the first-step ve…

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★ 10 cited

Lack of close-in, massive planets of main-sequence A-type stars from Kepler

Silvia Sabotta, Petr Kabath, Judith Korth +5

Some theories of planet formation and evolution predict that intermediate-mass stars host more hot Jupiters than Sun-like stars, others reach the conclusion that such objects are v…

astro-ph.EP2019

The role of small telescopes as a ground-based support for exoplanetary space missions

P. Kabath, M. Skarka, S. Sabotta +1

Small telescopes equiped with modern instrumentation are gaining on importance, especially, in the era of exoplanetary space missions such as TESS, PLATO and ARIEL. Crucial part of…

astro-ph.SR2019★ 63 cited

A possibly inflated planet around the bright, young star DS Tuc A

S. Benatti, D. Nardiello, L. Malavolta +13

The origin of the observed diversity of planetary system architectures is one of the main topic of the exoplanetary research. The detection of a statistically significant sample of…

astro-ph.EP2017★ 61 cited

K2-106, a system containing a metal-rich planet and a planet of lower density

E. W. Guenther, O. Barragan, F. Dai +42

Planets in the mass range from 2 to 15 MEarth are very diverse. Some of them have low densities, while others are very dense. By measuring the masses and radii, the mean densities,…