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20082024
most citedA White Dwarf catalogue from Gaia-DR2 and the Virtual Observatory

142 citations · 1.8k across the 36 of their papers we have counts for

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21 papers · 1 filter

astro-ph.SR2024★ 42 cited

Photometric segregation of dwarf and giant FGK stars using the SVO Filter Profile Service and photometric tools

Carlos Rodrigo, Patricia Cruz, John F. Aguilar +18

This paper is focused on the segregation of FGK dwarf and giant stars through narrow-band photometric data using the Spanish Virtual Observatory (SVO) Filter Profile Service and as…

astro-ph.SR2023★ 24 cited

White dwarf spectral type-temperature distribution from Gaia-DR3 and the Virtual Observatory

S. Torres, P. Cruz, R. Murillo-Ojeda +6

The characterization of white dwarf atmospheres is crucial for accurately deriving stellar parameters such as effective temperature, mass, and age. We aim to classify the populatio…

astro-ph.SR2023★ 50 cited

The Gaia-ESO Survey: homogenisation of stellar parameters and elemental abundances

A. Hourihane, P. Francois, C. C. Worley +59

The Gaia-ESO Survey is a public spectroscopic survey that has targeted stars covering all major components of the Milky Way from the end of 2011 to 2018, delivering i…

astro-ph.SR2022★ 133 cited

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

G. Gilmore, S. Randich, C. C. Worley +165

The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representat…

astro-ph.SR2022★ 19 cited

The Gaia-ESO Survey: The analysis of the hot-star spectra

R. Blomme, S. Daflon, M. Gebran +44

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that has collected, over a period of 6 years, spectra of ~ 10^5 stars. This survey provides not only the reduced sp…

astro-ph.SR2021★ 43 cited

The Gaia-ESO Survey: Target selection of open cluster stars

A. Bragaglia, E. Alfaro, E. Flaccomio +36

The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey with FLAMES@VLT. GES targeted in particular a large sample of open clusters (OCs) of all ages. The diffe…

astro-ph.SR2021★ 32 cited

Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution

E. Franciosini, E. Tognelli, S. Degl'Innocenti +24

Pre-main sequence models with inflated radii are needed to simultaneously reproduce the colour-magnitude diagram and the lithium depletion pattern in young open clusters. We tested…

astro-ph.SR2021★ 26 cited

The Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars

L. Magrini, R. Smiljanic, E. Franciosini +25

It has recently been suggested that all giant stars with mass below 2 suffer an episode of surface lithium enrichment between the tip of the red giant branch (RGB) and…

astro-ph.SR2021★ 43 cited

The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce

M. Baratella, V. D'Orazi, V. Sheminova +32

Young open clusters (t<200 Myr) have been observed to exhibit several peculiarities in their chemical compositions, from a slightly sub-solar iron content, super-solar abundances o…

astro-ph.SR2021★ 54 cited

The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field stars

L. Magrini, N. Lagarde, C. Charbonnel +42

We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from th…

astro-ph.SR2019★ 51 cited

Infrared-excess white dwarfs in the Gaia 100 pc sample

A. Rebassa-Mansergas, E. Solano, S. Xu +3

We analyse the 100pc Gaia white dwarf volume-limited sample by means of VOSA (Virtual Observatory SED Analyser) with the aim of identifying candidates for displaying infrared exces…

astro-ph.SR2019★ 47 cited

Random Forest identification of the thin disk, thick disk and halo Gaia-DR2 white dwarf population

S. Torres, C. Cantero, A. Rebassa-Mansergas +3

Gaia-DR2 has provided an unprecedented number of white dwarf candidates of our Galaxy. In particular, it is estimated that Gaia-DR2 has observed nearly 400,000 of these objects and…

astro-ph.SR2018★ 142 cited

A White Dwarf catalogue from Gaia-DR2 and the Virtual Observatory

F. M. Jiménez-Esteban, S. Torres, A. Rebassa-Mansergas +4

We present a catalogue of 73,221 white dwarf candidates extracted from the astrometric and photometric data of the recently published Gaia DR2 catalogue. White dwarfs were selected…

astro-ph.SR2017★ 57 cited

The Gaia-ESO Survey: Galactic evolution of sulphur and zinc

S. Duffau, E. Caffau, L. Sbordone +48

Due to their volatile nature, when sulfur and zinc are observed in external galaxies, their determined abundances represent the gas-phase abundances in the interstellar medium. Thi…

astro-ph.SR2016★ 31 cited

The Gaia-ESO Survey: the inner disk, intermediate-age open cluster Trumpler 23

J. C. Overbeek, E. D. Friel, P. Donati +33

Context: Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a Rgc ~6 kpc. It is in a crowded field very close to the Galactic plane and…

astro-ph.SR2016★ 37 cited

The Gaia-ESO Survey: Dynamical Analysis of the L1688 region in Ophiuchus

Elisabetta Rigliaco, B. Wilking, M. R. Meyer +25

The Gaia ESO Public Spectroscopic Survey (GES) is providing the astronomical community with high-precision measurements of many stellar parameters including radial velocities (RVs)…

astro-ph.SR2015★ 20 cited

The Gaia-ESO Survey: Catalogue of H emission stars

Gregor Traven, Tomaž Zwitter, Sophie Van Eck +18

We discuss the properties of H emission stars across the sample of 22035 spectra from the Gaia-ESO Survey internal data release, observed with the GIRAFFE instrument and largely…

astro-ph.SR2015★ 72 cited

Testing the chemical tagging technique with open clusters

S. Blanco-Cuaresma, C. Soubiran, U. Heiter +12

Context. Stars are born together from giant molecular clouds and, if we assume that the priors were chemically homogeneous and well-mixed, we expect them to share the same chemical…

astro-ph.SR2015★ 50 cited

The Gaia-ESO Survey: Discovery of a spatially extended low-mass population in the Vela OB2 association

G. G. Sacco, R. D. Jeffries, S. Randich +28

The nearby (distance~350-400 pc), rich Vela OB2 association, includes Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for inv…

astro-ph.SR2014★ 80 cited

The Gaia-ESO Survey: Stellar content and elemental abundances in the massive cluster NGC 6705

T. Cantat-Gaudin, A. Vallenari, S. Zaggia +52

Chemically inhomogeneous populations are observed in most globular clusters, but not in open clusters. Cluster mass seems to play a key role in the existence of multiple population…

astro-ph.SR2014★ 41 cited

The Gaia-ESO Survey: Properties of the intermediate age open cluster NGC 4815

E. D. Friel, P. Donati, A. Bragaglia +34

NGC 4815 is a populous ~500 Myr open cluster at a Galactocentric radius of 7 kpc observed in the first six months of the Gaia-ESO Survey. Located in the inner Galactic disk, NGC 48…