activity
20162026
most citedThe relationship between mono-abundance and mono-age stellar populations in the Milky Way disk

70 citations · 146 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Towards breaking the degeneracy between stellar ages and unresolved multiplicity

Friedrich Anders, Anna B. A. Queiroz, Sagar Malhotra +2

Stellar age is the central desirable parameter we need to disentangle different Galactic formation scenarios. Nevertheless, no stellar age dating method is completely model-indepen…

astro-ph.GA2026

Chemo-dynamical Analysis of a CNO-Enhanced Ultra Metal-poor Star (): Insights into Early Enrichment by Faint Population III Supernova

Guilherme Limberg, Vinicius M. Placco, Alexander P. Ji +10

We report an independent identification of the ultra metal-poor (UMP) star () DR3 $\texttt{source_id}$ 4795913112968206720 (GDR3_479591) in the miss…

astro-ph.EP2025★ 1 cited

Modelling the Milky Way's exoplanet population based on cosmological galaxy simulations

Chloé Padois, Daniel del Ser, Friedrich Anders +7

In this paper we aim to simulate realistic exoplanet populations across different regions of the MW by combining state-of-the-art cosmological simulations of our Galaxy with exopla…

astro-ph.CO2025★ 3 cited

The oldest Milky Way stars: New constraints on the age of the Universe and the Hubble constant

Elena Tomasetti, Cristina Chiappini, Samir Nepal +6

We exploit the most robust, old, and cosmology-independent age estimates of individual stars from Gaia DR3 to place a lower bound on the age of the Universe, . These constrain…

astro-ph.GA2025★ 8 cited

The Nineteenth Data Release of the Sloan Digital Sky Survey

SDSS Collaboration, Gautham Adamane Pallathadka, Mojgan Aghakhanloo +210

Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial…

astro-ph.GA2025★ 2 cited

The Spheroidal Bulge of the Milky Way: Chemodynamically Distinct from the Inner-Thick Disc and Bar

Samir Nepal, Cristina Chiappini, Angeles Pérez-Villegas +7

Studying the composition and origin of the inner region of our Galaxy -- the "Galactic bulge" -- is crucial for understanding the formation and evolution of the Milky Way and other…

astro-ph.GA2025

Early Co-formation of the Milky Way's Thin and Thick Disks at Redshift z > 2

Lais Borbolato, Silvia Rossi, Hélio D. Perottoni +8

The Milky Way serves as a template for understanding the formation and evolution of late-type massive disk galaxies since we can obtain detailed chemical and kinematic information…

astro-ph.GA2023

All-sky Kinematics and Chemistry of Monoceros Stellar Overdensity

Lais Borbolato, Hélio D. Perottoni, Silvia Rossi +7

We explore the kinematic and chemical properties of Monoceros stellar overdensity by combining data from 2MASS, WISE, APOGEE, and . Monoceros is a structure located to…

astro-ph.GA2020★ 62 cited

An all-sky proper motion map of the Sagittarius stream using Gaia DR2

T. Antoja, P. Ramos, C. Mateu +4

We aim to measure the proper motion along the Sagittarius stream that is the missing piece to determine its full 6D phase space coordinates. We conduct a blind search of over-densi…

astro-ph.GA2016★ 70 cited

The relationship between mono-abundance and mono-age stellar populations in the Milky Way disk

I. Minchev, M. Steinmetz, C. Chiappini +4

Studying the Milky Way disk structure using stars in narrow bins of [Fe/H] and [alpha/Fe] has recently been proposed as a powerful method to understand the Galactic thick and thin…