activity
20112026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 18.6k across the 151 of their papers we have counts for

collaborators

151 papers

astro-ph.GA2026

Reassessing the low- massive sequence stars in Gaia RVS

G. Nandakumar, G. Kordopatis, M. Schultheis +4

Recently, a chemically depleted young massive stellar population was identified using the spectroscopic catalogue of Gaia DR3. To explain its characteristics, a recent enhanced sta…

astro-ph.IM2025

Milky Way disc & Bulge in situ populations: ESO white paper - Expanding horizons call

M. Bergemann, G. Kordopatis, G. Casali +11

The formation and evolution of the Milky Way's disc, bar, and bulge remain fundamentally limited by the lack of a contiguous, Galaxy-wide, high-precision chemo-dynamical map. Key o…

astro-ph.GA2025

Mapping the Ages of Stars with Chemistry

Carlos Viscasillas Vázquez, Giada Casali, Laura Magrini +11

Chemical clocks, based on age-sensitive stellar abundance ratios, offer a powerful and scalable approach to reconstruct the formation history of the Milky Way. This white paper out…

astro-ph.SR2025

Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey

Nicholas Storm, Maria Bergemann, Tomasz Różański +9

We present the 4MOST-HR resolution Non-Local Thermal Equilibrium (NLTE) Payne artificial neural network (ANN), trained on new FGK spectra with 16 elements computed in NL…

astro-ph.GA2025

Supergiant GCIRS 22 in the Milky Way Nuclear Star Cluster: Revised alpha abundances

B. Thorsbro, S. Khalidy, R. M. Rich +7

Context: The chemical abundances of alpha-elements in Galactic Centre (GC) supergiants provide key insights into the chemical enrichment and star formation history of the Milky Way…

astro-ph.GA2025★ 1 cited

First large scale spatial and velocity patterns of local metal-rich stars in the Milky Way

Georges Kordopatis, Diane Feuillet, Christian Lehmann +4

(Abridged) The present-day spatial and kinematic distribution of stars in the Milky Way provides key constraints on its internal dynamics and evolutionary history. We select stars…

astro-ph.GA2025★ 7 cited

A Pristine-UNIONS view on the Galaxy: Kinematics of the distant spur feature of the Sagittarius stream traced by Blue Horizontal Branch stars

M. Bayer, E. Starkenburg, G. F. Thomas +14

Providing a detailed picture of the Sagittarius (Sgr) stream offers important constraints on the build-up of the Galactic halo as well as its gravitational potential at large radii…

astro-ph.GA2025★ 7 cited

Bar-spiral interaction produces radial migration and star formation bursts

Léa Marques, Ivan Minchev, Bridget Ratcliffe +8

Central bars and spirals are known to strongly impact the evolution of their host galaxies, both in terms of dynamics and star formation. Their typically different pattern speeds c…

astro-ph.GA2025★ 5 cited

The Pristine survey: XXVII. The extremely metal-poor stream C-19 stretches over more than 100 degrees

Zhen Yuan, Tadafumi Matsuno, Tatyana Sitnova +14

The discovery of the most metal-poor stream, C-19, provides us with a fossil record of a stellar structure born very soon after the Big Bang. In this work, we search for new C-19 m…

astro-ph.GA2024★ 2 cited

The Pristine survey. XXVI. Chemical abundances of subgiant stars of the extremelymetal-poor stream C-19

P. Bonifacio, E. Caffau, P. François +17

Context: The C-19 stellar stream is the most metal-poor stream known to date. While its width and velocity dispersion indicate a dwarf galaxy origin, its metallicity spread and abu…

astro-ph.SR2024★ 8 cited

Chemodynamic evolution of Sun-like stars in nearby moving groups

Christian Lehmann, Michael T. Murphy, Fan Liu +1

Sun-like stars are well represented in the solar neighbourhood but are currently under-utilised, with many studies of chemical and kinematic evolution focusing on red giants (which…

astro-ph.GA2024

Chemical Abundances in the Nuclear Star Cluster of the Milky Way: alpha-Element Trends and Their Similarities with the Inner Bulge

N. Ryde, G. Nandakumar, M. Schultheis +15

A chemical characterization of the Galactic Center is essential for understanding its formation and structural evolution. Trends of alpha-elements, such as Mg, Si, and Ca, serve as…

astro-ph.GA2024★ 6 cited

New stellar age estimates using SPInS based on Gaia DR3 photometry and LAMOST DR8 abundances

L. Casamiquela, D. R. Reese, Y. Lebreton +8

Reliable stellar age estimates are fundamental for testing several problems in modern astrophysics, in particular since they set the time scales of Galactic dynamical and chemical…

astro-ph.GA2024

An ancient system hidden in the Galactic plane?

Federico Sestito, Emma Fernandez-Alvar, Rebecca Brooks +19

We analyse high signal-to-noise ESPaDOnS/CFHT spectra of 20 very metal-poor stars (VMP; [Fe/H]~) in the solar neighbourhood (within kpc), selected to be on planar or…

astro-ph.GA2024

The Pristine survey XXIV: The Galactic underdogs -- Dynamic tales of a Milky Way metal-poor population

Isaure González Rivera de La Vernhe, Vanessa Hill, Georges Kordopatis +12

Through the chemodynamical characterisation of metal-poor stars, one can efficiently probe the early history of the Milky Way. We aim at decontaminating a sample of 3M giant…

astro-ph.GA2024★ 11 cited

The Pristine Inner Galaxy Survey (PIGS) IX. The largest detailed chemical analysis of very metal-poor stars in the Sagittarius dwarf galaxy

Federico Sestito, Sara Vitali, Paula Jofre +16

The most metal-poor stars provide valuable insights into the early chemical enrichment history of a system, carrying the chemical imprints of the first generations of supernovae. T…

astro-ph.GA2024★ 8 cited

Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE

Christian Lehmann, Sofia Feltzing, Diane Feuillet +1

Making use of the APOGEE DR17 catalogue with high quality data for 143,509 red giant branch stars we explore the strength of different mechanisms that causes a star to radially mig…

astro-ph.GA2024★ 5 cited

A Wide Metallicity Range for Gyr-old Stars in the Nuclear Star Cluster

Brian Thorsbro, Rebecca Forsberg, Georges Kordopatis +6

We report metallicities for three Gyr-old stars in the Milky Way nuclear star cluster (NSC) using high-resolution near-infrared spectroscopy. We derive effective temperatures…

astro-ph.GA2024★ 129 cited

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry

Gaia Collaboration, P. Panuzzo, T. Mazeh +412

Gravitational waves from black-hole merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected base…

astro-ph.IM2024★ 12 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

astro-ph.GA2024★ 9 cited

SpectroTranslator: a deep-neural network algorithm to homogenize spectroscopic parameters

G. F. Thomas, G. Battaglia, F. Gran +8

The emergence of large spectroscopic surveys requires homogenising on the same scale the quantities they measure in order to increase their scientific legacy. We developed the Spec…

astro-ph.GA2024★ 15 cited

On the metal-poor edge of the Milky Way "thin disc"

Emma Fernández-Alvar, Georges Kordopatis, Vanessa Hill +9

The emergence of the disc in our Galaxy and the relation of the thick and thin disc formation and evolution is still a matter of debate. The chemo-dynamical characterization of dis…

astro-ph.GA2023

Gaia Focused Product Release: Spatial distribution of two diffuse interstellar bands

Gaia Collaboration, M. Schultheis, H. Zhao +15

Diffuse interstellar bands (DIBs) are absorption features seen in optical and infrared spectra of stars that are probably caused by large and complex molecules in the ISM. Here we…

astro-ph.GA2023★ 10 cited

Could very low-metallicity stars with rotation-dominated orbits have been shepherded by the bar?

Zhen Yuan, Chengdong Li, Nicolas F. Martin +11

The most metal-poor stars (e.g. [Fe/H] ) are the ancient fossils from the early assembly epoch of our Galaxy, very likely before the formation of the thick disc. Recent s…