activity
20172021
most citedA candidate super-Earth planet orbiting near the snow line of Barnard's star

142 citations · 674 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2021★ 74 cited

Rapid contraction of giant planets orbiting the 20 million-years old star V1298 Tau

A. Suárez Mascareño, M. Damasso, N. Lodieu +41

Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about…

astro-ph.EP2021★ 11 cited

HADES RV Programme with HARPS-N at TNG XIII. A sub-Neptune around the M dwarf GJ 720 A

E. González-Álvarez, A. Petralia, G. Micela +21

Context. The high number of super-Earth and Earth-like planets in the habitable zone (HZ) detected around M-dwarf stars in the last years has revealed these stellar objects to be t…

astro-ph.SR2020★ 76 cited

HADES RV Programme with HARPS-N at TNG XII. The abundance signature of M dwarf stars with planets

J. Maldonado, G. Micela, M. Baratella +27

Most of our current knowledge on planet formation is still based on the analysis of main-sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M-dwa…

astro-ph.SR2020★ 37 cited

The solar gravitational redshift from HARPS-LFC Moon spectra. A test of the General Theory of Relativity

J. I. González Hernández, R. Rebolo, L. Pasquini +15

The General Theory of Relativity predicts the redshift of spectral lines in the solar photosphere, as a consequence of the gravitational potential of the Sun. This effect can be me…

astro-ph.IM2020★ 57 cited

A crucial test for astronomical spectrograph calibration with frequency combs

Rafael A. Probst, Dinko Milaković, Borja Toledo-Padrón +23

Laser frequency combs (LFCs) are well on their way to becoming the next-generation calibration sources for precision astronomical spectroscopy. This development is considered key i…

astro-ph.SR2020★ 26 cited

A detailed non-LTE analysis of LB-1: Revised parameters and surface abundances

S. Simón-Díaz, J. Maíz Apellániz, D. J. Lennon +8

LB-1 has recently been proposed to be a binary system at 4 kpc consisting of a B star of 8 Msol and a massive stellar black hole of 70 Msol. This finding challenges our current the…

astro-ph.EP2019★ 33 cited

Gliese 49: Activity evolution and detection of a super-Earth

M Perger, G Scandariato, I Ribas +40

Small planets around low-mass stars often show orbital periods in a range that corresponds to the temperate zones of their host stars which are therefore of prime interest for plan…

astro-ph.SR2019★ 20 cited

HADES RV Programme with HARPS-N at TNG. X. The non-saturated regime of the stellar activity-rotation relationship for M-Dwarfs

E. González-Álvarez, G. Micela, J. Maldonado +22

Aims. We aim to extend the relationship between X-ray luminosity (Lx) and rotation period (Prot) found for main-sequence FGK stars and test whether it also holds for early-M dwarfs…

astro-ph.EP2019★ 24 cited

HADES RV program with HARPS-N at TNG. IX. A super-Earth around the M dwarf Gl686

L. Affer, M. Damasso, G. Micela +25

The HArps-n red Dwarf Exoplanet Survey is providing a major contribution to the widening of the current statistics of low-mass planets, through the in-depth analysis of precise rad…

astro-ph.SR2018★ 3 cited

High-resolution spectroscopy of Boyajian's star during optical dimming events

M. J. Martínez González, C. González-Fernández, A. Asensio Ramos +13

Boyajian's star is an apparently normal main sequence F-type star with a very unusual light curve. The dipping activity of the star, discovered during the Kepler mission, presents…

astro-ph.EP2018★ 142 cited

A candidate super-Earth planet orbiting near the snow line of Barnard's star

I. Ribas, M. Tuomi, A. Reiners +60

At a distance of 1.8 parsecs, Barnard's star (Gl 699) is a red dwarf with the largest apparent motion of any known stellar object. It is the closest single star to the Sun, second…

astro-ph.EP2018★ 40 cited

The HADES RV Programme with HARPS-N@TNG VIII. Gl15A: A multiple wide planetary system sculpted by binary interaction

M. Pinamonti, M. Damasso, F. Marzari +28

We present 20 years of radial velocity (RV) measurements of the M1 dwarf Gl15A, combining 5 years of intensive RV monitoring with the HARPS-N spectrograph with 15 years of archival…

astro-ph.SR2017★ 78 cited

HADES RV Programme with HARPS-N at TNG. VII. Rotation and activity of M-Dwarfs from time-series high-resolution spectroscopy of chromospheric indicators

A. Suárez Mascareño, R. Rebolo, J. I. González Hernández +28

We aim to investigate the presence of signatures of magnetic cycles and rotation on a sample of 71 early M-dwarfs from the HADES RV programme using high-resolution time-series spec…

astro-ph.SR2017★ 19 cited

HADES RV Programme with HARPS-N at TNG VI. GJ 3942 b behind dominant activity signals

M. Perger, I. Ribas, M. Damasso +29

Short- to mid-term magnetic phenomena on the stellar surface of M-type stars cannot only resemble the effects of planets in radial velocity data, but also may hide them. We analyze…

astro-ph.EP2017★ 34 cited

HADES RV Programme with HARPS-N at TNG: V. A super-Earth on the inner edge of the habitable zone of the nearby M-dwarf GJ 625

A. Suárez Mascareño, J. I. González Hernández, R. Rebolo +27

We report the discovery of a super-Earth orbiting at the inner edge of the habitable zone of the star GJ 625 based on the analysis of the radial-velocity (RV) time series from the…