activity
20132026
most citedGaia FGK Benchmark Stars - Metallicity

314 citations · 494 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

Comparing phylogenetic trees of stars with spectral graph distances

Theosamuele Signor, Matias Neto, Paula Jofré +9

Phylogenetic trees offer a hierarchical representation of chemical similarities among stars, from which their evolutionary histories can, in principle, be reconstructed. Simulation…

astro-ph.GA2026

The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper

SDSS Collaboration, Mojgan Aghakhanloo, David Aguilar +273

This paper presents the twentieth data release (DR20) from the Sloan Digital Sky Survey, the third data release of its fifth generation (SDSS-V). SDSS-V is a panoptic spectroscopy…

astro-ph.SR2026

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis

Pierre F. L. Maxted, Nicholas Storm, Andreas J. Korn +7

AI Phe is an eclipsing binary star with an orbital period of 24.6 days for which the surface gravity and effective temperature are known from direct measurements to very high preci…

astro-ph.SR2024★ 2 cited

Full abundance study of two newly discovered barium giants

Sara Vitali, Ana Escorza, Ditte Slumstrup +1

Barium (Ba) stars are chemically peculiar stars that show enhanced surface abundances of heavy elements produced by the slow-neutron-capture process, the so-called s-process. These…

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.GA2023★ 1 cited

Assembling a high-precision abundance catalogue of solar twins in GALAH for phylogenetic studies

Kurt Walsen, Paula Jofré, Sven Buder +13

Stellar chemical abundances have proved themselves a key source of information for understanding the evolution of the Milky Way, and the scale of major stellar surveys such as GALA…

astro-ph.SR2022★ 3 cited

Discovery of a brown dwarf with quasi-spherical mass-loss

Dary A. Ruíz-Rodríguez, Lucas A. Cieza, Simon Casassus +14

We report the serendipitous discovery of an elliptical shell of CO associated with the faint stellar object SSTc2d J163134.1-24006 as part of the "Ophiuchus Disk Survey Employing A…

astro-ph.SR2021★ 9 cited

Fundamental stellar parameters of benchmark stars from CHARA interferometry -- III. Giant and subgiant stars

I. Karovicova, T. R. White, T. Nordlander +3

Large spectroscopic surveys of the Milky Way need to be calibrated against a sample of benchmark stars to ensure the reliable determination of atmospheric parameters. We present ne…

astro-ph.SR2021★ 14 cited

Fundamental stellar parameters of benchmark stars from CHARA interferometry -- II. Dwarf stars

I. Karovicova, T. R. White, T. Nordlander +3

Stellar models applied to large stellar surveys of the Milky Way need to be properly tested against a sample of stars with highly reliable fundamental stellar parameters. We have e…

astro-ph.GA2021

Two sequences in the age-metallicity relation as seen from [C/N] abundances in APOGEE

Paula Jofre

The age-metallicity relation is fundamental to study the formation and evolution of the disk. Observations have shown that this relation has a large scatter which can not be explai…

astro-ph.SR2021★ 16 cited

The consistency of chemical clocks among coeval stars

Francisca Espinoza-Rojas, Julio Chanamé, Paula Jofré +1

The abundance ratios of some chemical species have been found to correlate with stellar age, leading to the possibility of using stellar atmospheric abundances as stellar age indic…

astro-ph.EP2021★ 35 cited

Host-star and exoplanet compositions: a pilot study usinga wide binary with a polluted white dwarf

Amy Bonsor, Paula Jofre, Oliver Shorttle +3

Planets and stars ultimately form out of the collapse of the same cloud of gas. Whilst planets, and planetary bodies, readily loose volatiles, a common hypothesis is that they reta…

astro-ph.GA2020★ 11 cited

Using heritability of stellar chemistry to reveal the history of the Milky Way

Holly Jackson, Paula Jofre, Keaghan Yaxley +3

Since chemical abundances are inherited between generations of stars, we use them to trace the evolutionary history of our Galaxy. We present a robust methodology for creating a ph…

astro-ph.SR2019★ 9 cited

Traits for chemical evolution in solar twins: Trends of neutron-capture elements with stellar age

Paula Jofre, Holly Jackson, Marcelo Tucci Maia

The physical processes driving chemical evolution in the Milky Way can be probed using the distribution of abundances in low-mass FGK type stars in space phase at different times.…

astro-ph.GA2017★ 1 cited

Galactic Phylogenetics

P. Jofre, P. Das

Phylogenetics is a widely used concept in evolutionary biology. It is the reconstruction of evolutionary history by building trees that represent branching patterns and sequences.…

astro-ph.GA2016★ 47 cited

Cosmic phylogeny: reconstructing the chemical history of the solar neighbourhood with an evolutionary tree

Paula Jofre, Payel Das, Jaume Bertranpetit +1

Using 17 chemical elements as a proxy for stellar DNA, we present a full phylogenetic study of stars in the solar neighbourhood. This entails applying a clustering technique that i…

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.GA2013★ 314 cited

Gaia FGK Benchmark Stars - Metallicity

Paula Jofre, U. Heiter, C. Soubiran +22

To calibrate automatic pipelines that determine atmospheric parameters of stars, one needs a sample of stars -- ``benchmark stars'' -- with well defined parameters to be used as a…