activity
20212024
most citedThe detailed chemical abundance patterns of accreted halo stars from the optical to infrared

38 citations · 90 across the 9 of their papers we have counts for

collaborators

9 papers

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★ 2 cited

The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates

Danielle de Brito Silva, Paula Jofré, Clare Worley +2

The Milky Way is a mosaic of stars from different origins. In particular, metal-poor accreted star candidates offer a unique opportunity to better understand the accretion history…

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.HE2024★ 22 cited

Early emission lines in SN 2024ggi revealed by high-resolution spectroscopy

Thallis Pessi, Régis Cartier, Emilio Hueichapan +6

We present an analysis of very early high-resolution spectroscopic observations of the Type II supernova (SN) 2024ggi, a nearby SN that occurred in the galaxy NGC 3621 at a distanc…

astro-ph.GA2023★ 1 cited

On the evolutionary history of a simulated disc galaxy as seen by phylogenetic trees

Danielle de Brito Silva, Paula Jofré, Patricia B. Tissera +12

Phylogenetic methods have long been used in biology, and more recently have been extended to other fields - for example, linguistics and technology - to study evolutionary historie…

astro-ph.SR2023

Gaia FGK Benchmark Stars: fundamental Teff and log g of the third version

Caroline Soubiran, Orlagh Creevey, Nadege Lagarde +8

Context. Large spectroscopic surveys devoted to the study of the Milky Way, including Gaia, use automated pipelines to massively determine the atmospheric parameters of millions of…

astro-ph.GA2022★ 11 cited

Unraveling UBC 274: a morphological, kinematical and chemical analysis of a disrupting open cluster

L. Casamiquela, J. Olivares, Y. Tarricq +8

We do a morphological, kinematic and chemical analysis of the disrupting cluster UBC 274 (2.5 Gyr, pc) to study its global properties. We use HDBSCAN to obtain a new membe…

astro-ph.SR2022★ 38 cited

The detailed chemical abundance patterns of accreted halo stars from the optical to infrared

Andreia Carrillo, Keith Hawkins, Paula Jofré +3

Understanding the assembly of our Galaxy requires us to also characterize the systems that helped build it. In this work, we accomplish this by exploring the chemistry of accreted…

astro-ph.GA2021★ 5 cited

J-PLUS: Detecting and studying extragalactic globular clusters -- the case of NGC 1023

Danielle de Brito Silva, Paula Coelho, Arianna Cortesi +19

Extragalactic globular clusters (GCs) are key objects for studying the history of galaxies. The arrival of wide-field surveys such as the Javalambre Photometric Local Universe Surv…