activity
20092026
most citedThe PLATO 2.0 Mission

1.3k citations · 13.9k across the 272 of their papers we have counts for

collaborators
Showing 2014Show all

15 papers · 1 filter

astro-ph.SR2014★ 148 cited

Li abundances in F stars: planets, rotation and galactic evolution

E. Delgado Mena, S. Bertrán de Lis, V. Zh. Adibekyan +7

We find that hot jupiter host stars within the T range 5900-6300K show lower Li abundances, by 0.14 dex, than stars without detected planets. This offset has a signi…

astro-ph.EP2014★ 52 cited

Revisiting the correlation between stellar activity and planetary surface gravity

P. Figueira, M. Oshagh, V. Zh. Adibekyan +1

Aims: We re-evaluate the correlation between planetary surface gravity and stellar host activity as measured by the index log(). This correlation, previously identified by…

astro-ph.SR2014

Stars with and without planets: Where do they come from?

V. Zh. Adibekyan, J. I. Gonzalez Hernandez, E. Delgado Mena +5

A long and thorough investigation of chemical abundances of planet-hosting stars that lasted for more than a decade has finally beared fruit. We explore a sample of 148 solar-like…

astro-ph.SR2014★ 104 cited

Correcting the spectroscopic surface gravity using transits and asteroseismology. No significant effect on temperatures or metallicities with ARES+MOOG in LTE

A. Mortier, S. G. Sousa, V. Zh. Adibekyan +2

Precise stellar parameters are crucial for several reasons, amongst which are the precise characterization of orbiting exoplanets and the correct determination of galactic chemical…

astro-ph.EP2014★ 32 cited

Exoplanet hosts reveal lithium depletion: Results from a homogeneous statistical analysis

P. Figueira, J. P. Faria, E. Delgado-Mena +4

Aims. We study the impact of the presence of planets on the lithium abundance of host stars and evaluate the previous claim that planet hosts exhibit lithium depletion when compare…

astro-ph.SR2014★ 227 cited

Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

R. Smiljanic, A. J. Korn, M. Bergemann +99

The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-t…

astro-ph.SR2014★ 41 cited

Spectroscopic parameters for solar-type stars with moderate/high rotation. New parameters for 10 planet-hosts

M. Tsantaki, S. G. Sousa, N. C. Santos +5

Planetary studies demand precise and accurate stellar parameters as input to infer the planetary properties. Different methods often provide different results that could lead to bi…

astro-ph.GA2014★ 36 cited

Supernovae and their host galaxies - II. The relative frequencies of supernovae types in spirals

A. A. Hakobyan, T. A. Nazaryan, V. Zh. Adibekyan +8

We present an analysis of the relative frequencies of different supernova (SN) types in spirals with various morphologies and in barred or unbarred galaxies. We use a well-defined…

astro-ph.SR2014★ 42 cited

The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region

L. Spina, S. Randich, F. Palla +37

Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun…

astro-ph.SR2014★ 36 cited

The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster Gamma Velorum

L. Spina, S. Randich, F. Palla +36

Knowledge of the abundance distribution of star forming regions and young clusters is critical to investigate a variety of issues, from triggered star formation and chemical enrich…

astro-ph.EP2014★ 120 cited

The HARPS search for southern extra-solar planets XXXV. The interesting case of HD41248: stellar activity, no planets?

N. C. Santos, A. Mortier, J. P. Faria +21

The search for planets orbiting metal-poor stars is of uttermost importance for our understanding of the planet formation models. However, no dedicated searches have been conducted…

astro-ph.SR2014★ 97 cited

On the origin of stars with and without planets. Tc trends and clues to Galactic evolution

V. Zh. Adibekyan, J. I. Gonzalez Hernandez, E. Delgado Mena +5

We explore a sample of 148 solar-like stars to search for a possible correlation between the slopes of the abundance trends versus condensation temperature (known as the Tc slope)…

astro-ph.GA2014★ 241 cited

The Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

A. Recio-Blanco, P. de Laverny, G. Kordopatis +36

(Abridged) We have used the atmospheric parameters, [alpha/Fe] abundances and radial velocities, determined from the Gaia-ESO Survey GIRAFFE spectra of FGK-type stars (iDR1), to pr…

astro-ph.GA2014★ 12 cited

Searching for solar siblings among the HARPS data

S. F. A. Batista, V. Zh. Adibekyan, S. G. Sousa +3

The search for the solar siblings has been particularly fruitful in the last few years. Until now, there are four plausible candidates pointed out in the literature: HIP21158, HIP8…

astro-ph.HE2014

Study of unconfirmed supernovae

L. S. Aramyan, A. R. Petrosian, A. A. Hakobyan +5

We study the nature of 39 unconfirmed supernovae (SNe) from the sky area covered by Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8), using available photometric and imaging da…