activity
20162026
most citedThe CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars

253 citations · 4k across the 80 of their papers we have counts for

collaborators
Showing 2020 · astro-ph.SRShow all

5 papers · 2 filters

astro-ph.SR2020★ 25 cited

The CARMENES search for exoplanets around M dwarfs: Rubidium abundances in nearby cool stars

C. Abia, H. M. Tabernero, S. A. Korotin +25

In this study, abundances of the neutron-capture elements Rb, Sr, and Zr are derived, for the first time, in a sample of nearby M dwarfs. We focus on stars in the metallicity range…

astro-ph.SR2020★ 40 cited

The CARMENES search for exoplanets around M dwarfs -- A deep learning approach to determine fundamental parameters of target stars

V. M. Passegger, A. Bello-García, J. Ordieres-Meré +26

Existing and upcoming instrumentation is collecting large amounts of astrophysical data, which require efficient and fast analysis techniques. We present a deep neural network arch…

astro-ph.SR2020★ 43 cited

The CARMENES search for exoplanets around M dwarfs: Convective shift and starspot constraints from chromatic radial velocities

D. Baroch, J. C. Morales, I. Ribas +26

Context. Variability caused by stellar activity represents a challenge to the discovery and characterization of terrestrial exoplanets and complicates the interpretation of atmosph…

astro-ph.SR2020★ 3 cited

The CARMENES search for exoplanets around M dwarfs. Variability of the He I line at 10830 Å

B. Fuhrmeister, S. Czesla, L. Hildebrandt +23

The He I infrared (IR) triplet at 10830 Åis known as an activity indicator in solar-type stars and has become a primary diagnostic in exoplanetary transmission spectroscopy. He I l…

astro-ph.SR2020★ 7 cited

The CARMENES search for exoplanets around M dwarfs. The He I infrared triplet lines in PHOENIX models of M2-3 V stars

D. Hintz, B. Fuhrmeister, S. Czesla +25

The He I infrared (IR) line at a vacuum wavelength of 10833 A is a diagnostic for the investigation of atmospheres of stars and planets orbiting them. For the first time, we study…