activity
20042026
most citedA terrestrial planet candidate in a temperate orbit around Proxima Centauri

1.3k citations · 9k across the 195 of their papers we have counts for

collaborators
Showing 2018Show all

10 papers · 1 filter

astro-ph.EP2018★ 22 cited

Detection and characterization of an ultra-dense sub-Neptune planet orbiting the Sun-like star HD 119130

R. Luque, G. Nowak, E. Pallé +51

We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. HD 119130 b is a warm sub-Neptune on a 17-d orbit aroun…

astro-ph.EP2018★ 158 cited

Detection of He I Å absorption on HD 189733 b with CARMENES high-resolution transmission spectroscopy

M. Salz, S. Czesla, P. C. Schneider +35

We present three transit observations of HD 189733 b obtained with the high-resolution spectrograph CARMENES at Calar Alto. A strong absorption signal is detected in the near-infra…

astro-ph.SR2018★ 27 cited

Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle

B. Toledo-Padrón, J. I. González Hernández, C. Rodríguez-López +58

The search for Earth-like planets around late-type stars using ultra-stable spectrographs requires a very precise characterization of the stellar activity and the magnetic cycle of…

astro-ph.EP2018★ 81 cited

Multiple water band detections in the CARMENES near-infrared transmission spectrum of HD 189733 b

F. J. Alonso-Floriano, A. Sánchez-López, I. A. G. Snellen +27

Aims: We explore the capabilities of CARMENES for characterizing hot-Jupiter atmospheres by targeting multiple water bands, in particular, those at 1.15 and 1.4 m. Hubble Space…

astro-ph.SR2018★ 46 cited

The CARMENES search for exoplanets around M dwarfs: Nine new double-line spectroscopic binary stars

D. Baroch, J. C. Morales, I. Ribas +27

Context. The CARMENES spectrograph is surveying ~300 M dwarf stars in search for exoplanets. Among the target stars, spectroscopic binary systems have been discovered, which can be…

astro-ph.EP2018★ 50 cited

The CARMENES search for exoplanets around M dwarfs. A Neptune-mass planet traversing the habitable zone around HD 180617

A. Kaminski, T. Trifonov, J. A. Caballero +37

Despite their activity, low-mass stars are of particular importance for the search of exoplanets by the means of Doppler spectroscopy, as planets with lower masses become detectabl…

astro-ph.EP2018★ 27 cited

Detection and Doppler monitoring of EPIC 246471491, a system of four transiting planets smaller than Neptune

E. Palle, G. Nowak, R. Luque +43

The Kepler extended mission, also known as K2, has provided the community with a wealth of planetary candidates that orbit stars typically much brighter than the targets of the ori…

astro-ph.EP2018★ 91 cited

The CARMENES search for exoplanets around M dwarfs: A low-mass planet in the temperate zone of the nearby K2-18

Paula Sarkis, Thomas Henning, Martin Kürster +22

K2-18 is a nearby M2.5 dwarf, located at 34 pc and hosting a transiting planet which was first discovered by the {\it K2} mission and later confirmed with {\it Spitzer Space Telesc…

astro-ph.SR2018★ 71 cited

The CARMENES search for exoplanets around M dwarfs: Radial-velocity variations of active stars in visual-channel spectra

L. Tal-Or, M. Zechmeister, A. Reiners +22

Previous simulations predicted the activity-induced radial-velocity (RV) variations of M dwarfs to range from cm/s to km/s, depending on various stellar and activit…

astro-ph.SR2018★ 25 cited

The CARMENES search for exoplanets around M dwarfs: Wing asymmetries of H, Na I D, and He I lines

B. Fuhrmeister, S. Czesla, J. H. M. M. Schmitt +13

Stellar activity is ubiquitously encountered in M dwarfs and often characterised by the H line. In the most active M dwarfs, H is found in emission, sometimes with a complex…