activity
20172026
most citedThe Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

681 citations · 3k across the 53 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

33 papers · 1 filter

astro-ph.GA2026

A two-stage settling of the Milky Way disk revealed by precise ChronoGal ages

David Mirabal, Carme Gallart, Tomás Ruiz-Lara +9

The spatial distribution of Galactic disk stars of different ages and metallicities encodes its dynamical evolution history and formation pathways. The lack of precise ages for lar…

astro-ph.GA2026

Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream

Camila Navarrete, Álvaro Rojas-Arriagada, Andrés E. Piatti +8

The formation, extension, and morphology of extra-tidal stars around globular clusters depend on the internal kinematics of the host cluster and the Galactic potential. Tracing the…

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.GA2026★ 1 cited

Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration

Takuji Tsujimoto, Daisuke Taniguchi, Alejandra Recio-Blanco +2

Solar twins are among the most powerful tracers of Galactic disk evolution owing to their unique property of sharing nearly solar metallicities ([Fe/H] ~ 0) while spanning a wide r…

astro-ph.GA2025

3D extinction maps of the Milky Way disc from Gaia GSP-Spec parameters

M. Barbillon, A. Recio-Blanco, P. de Laverny +1

3D maps of interstellar dust are crucial for understanding the structure of the Milky Way interstellar medium to apply correction to astrophysical observations affected by dust. We…

astro-ph.GA2025★ 1 cited

Caveats about measuring carbon abundances in stars using the CH band

Pablo Santos-Peral, Patricia Sánchez-Blázquez, Alejandro Vazdekis +4

Deriving accurate carbon abundance estimates for a wide variety of stars is still complex due to the difficulties in properly measuring it from atomic and molecular lines. The aim…

astro-ph.GA2024★ 2 cited

Signatures of simulated spiral arms on radial actions

P. A. Palicio, A. Recio-Blanco, T. Tepper-Garcia +7

Among the various implications of the spiral arms, it has been observed in the Milky Way disc that the distribution of radial actions from the Gaia Data Release 3 exhibits structur…

astro-ph.GA2024★ 10 cited

Constraints on the history of Galactic spiral arms revealed by Gaia GSP-Spec alpha-elements

M. Barbillon, A. Recio-Blanco, E. Poggio +4

The distribution of chemical elements in the Galactic disc can reveal fundamental clues on the physical processes that led to the current configuration of our Galaxy. We map chemic…

astro-ph.GA2024★ 20 cited

The Great Wave: Evidence of a large-scale vertical corrugation propagating outwards in the Galactic disc

E. Poggio, S. Khanna, R. Drimmel +6

We analyse the three-dimensional structure and kinematics of two samples of young stars in the Galactic disc, containing respectively young giants (17000 stars out to he…

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.GA2024★ 11 cited

Double Red Giant Branch and Red Clump features of Galactic disc stellar populations with Gaia GSPspec

Alejandra Recio-Blanco, P. de Laverny, P. A. Palicio +4

To disentangle the different competing physical processes at play in Galactic evolution, a detailed chrono chemicalkinematical, and dynamical characterisation of the disc bimodalit…

astro-ph.GA2023★ 17 cited

2D chemical evolution models II. Effects of multiple spiral arm patterns on O, Eu, Fe and Ba abundance gradients

E. Spitoni, G. Cescutti, A. Recio-Blanco +7

According to observations and numerical simulations, the Milky Way could exhibit several spiral arm modes with multiple pattern speeds, wherein the slower patterns are located at l…

astro-ph.GA2023★ 7 cited

Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars

Gaia Collaboration, A. Krone-Martins, C. Ducourant +398

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space mission covers the entire sky with the unprecedented resolution of " in the optical, ma…

astro-ph.GA2023★ 17 cited

Analytic solution of Chemical Evolution Models with Type Ia SNe

P. A. Palicio, E. Spitoni, A. Recio-Blanco +3

Context: In the last years, a significant number of works have focused on finding analytic solutions for the chemical enrichment models of galactic systems, including the Milky Way…

astro-ph.GA2023★ 5 cited

Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances

Pablo Santos-Peral, Patricia Sánchez-Blázquez, Alexandre Vazdekis +1

The X-shooter Spectral Library (XSL) is a large empirical stellar library used as a benchmark for the development of stellar population models. The inclusion of -elements abunda…

astro-ph.GA2022★ 27 cited

Spiral-like features in the disc revealed by Gaia DR3 radial actions

P. A. Palicio, A. Recio-Blanco, E. Poggio +3

We aim to explore the actions of the new Gaia DR3 astrometry to find structures in the Galactic disc. We compute the actions and the orbital parameters of the Gaia DR3 stars with f…

astro-ph.GA2022★ 21 cited

The cerium content of the Milky Way as revealed by Gaia DR3 GSP-Spec abundances

G. Contursi, P. de Laverny, A. Recio-Blanco +12

The recent Gaia Third Data Release contains a homogeneous analysis of millions of high-quality Radial Velocity Spectrometer (RVS) stellar spectra by the GSP-Spec module. This led t…

astro-ph.GA2022★ 83 cited

Gaia DR3: Apsis III -- Non-stellar content and source classification

L. Delchambre, C. A. L. Bailer-Jones, I. Bellas-Velidis +78

Context. As part of the third Gaia data release, we present the contributions of the non-stellar and classification modules from the eighth coordination unit (CU8) of the Data Proc…

astro-ph.GA2022★ 58 cited

Stellar ages, masses, extinctions and orbital parameters based on spectroscopic parameters of Gaia DR3

G. Kordopatis, M. Schultheis, P. J. McMillan +13

Gaia DR3 provides radial velocities for 33 million stars and spectroscopically derived atmospheric parameters for more than five million targets. When combined with the astrometric…

astro-ph.GA2022★ 223 cited

Gaia Data Release 3: Astrophysical parameters inference system (Apsis) I -- methods and content overview

O. L. Creevey, R. Sordo, F. Pailler +86

Gaia Data Release 3 contains a wealth of new data products for the community. Astrophysical parameters are a major component of this release. They were produced by the Astrophysica…

astro-ph.GA2022★ 252 cited

Gaia Data Release 3: Analysis of RVS spectra using the General Stellar Parametriser from spectroscopy

A. Recio-Blanco, P. de Laverny, P. A. Palicio +77

The chemo-physical parametrisation of stellar spectra is essential for understanding the nature and evolution of stars and of Galactic stellar populations. Gaia DR3 contains the pa…

astro-ph.GA2022★ 66 cited

Gaia Data Release 3: Chemical cartography of the Milky Way

Gaia Collaboration, A. Recio-Blanco, G. Kordopatis +447

Gaia DR3 opens a new era of all-sky spectral analysis of stellar populations thanks to the nearly 5.6 million stars observed by the RVS and parametrised by the GSP-spec module. The…

astro-ph.GA2022★ 40 cited

The chemical signature of the Galactic spiral arms revealed by Gaia DR3

E. Poggio, A. Recio-Blanco, P. A. Palicio +8

Taking advantage of the recent Gaia Data Release 3 (DR3), we map chemical inhomogeneities in the Milky Way's disc out to a distance of 4 kpc from the Sun, using different sa…

astro-ph.GA2022★ 48 cited

Beyond the two-infall model I. Indications for a recent gas infall with Gaia DR3 chemical abundances

E. Spitoni, A. Recio-Blanco, P. de Laverny +7

The recent Gaia Data Release 3 (DR3) represents an unparalleled revolution in Galactic Archaeology, providing us with numerous radial velocities chemical abundances for millions of…