activity
20152021
most citedChemical abundances of 1111 FGK stars from the HARPS GTO planet search program II: Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd and Eu

212 citations · 853 across the 16 of their papers we have counts for

collaborators

21 papers

astro-ph.SR202121 cited

The homogeneous characterisation of Ariel host stars

C. Danielski, A. Brucalassi, S. Benatti +20

The Ariel mission will characterise the chemical and thermal properties of the atmospheres of about a thousand exoplanets transiting their host star(s). The observation of such a l…

astro-ph.IM202127 cited

Ariel: Enabling planetary science across light-years

Giovanna Tinetti, Paul Eccleston, Carole Haswell +313

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. Durin…

astro-ph.EP20217 cited

Determination of stellar parameters for Ariel targets: a comparison analysis between different spectroscopic methods

A. Brucalassi, M. Tsantaki, L. Magrini +9

Ariel has been selected as the next ESA M4 science mission and it is expected to be launched in 2028. During its 4-year mission, Ariel will observe the atmospheres of a large and d…

astro-ph.SR2020

Benchmark stars, benchmark spectrographs: Detailed spectroscopic comparison of ESPRESSO, PEPSI, and HARPS data for Gaia benchmark stars

V. Adibekyan, S. G. Sousa, N. C. Santos +14

Gaia benchmark stars are selected to be calibration stars for different spectroscopic surveys. Very high-quality and homogeneous spectroscopic data for these stars are therefore re…

astro-ph.SR202035 cited

The Gaia-ESO Survey: Galactic evolution of lithium at high metallicity

S. Randich, L. Pasquini, E. Franciosini +20

Reconstructing the Galactic evolution of lithium (Li) is the main tool used to constrain the source(s) of Li enrichment in the Galaxy. Recent results have suggested a decline in Li…

astro-ph.GA202088 cited

The Gaia-ESO survey: the non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

G. Casali, L. Spina, L. Magrini +36

In the era of large spectroscopic surveys, massive databases of high-quality spectra provide tools to outline a new picture of our Galaxy. In this framework, an important piece of…