activity
20202025
most citedThe GALAH Survey: Non-LTE departure coefficients for large spectroscopic surveys

105 citations · 193 across the 7 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2025★ 4 cited

A 3D view of dwarf galaxies with Gaia and VLT/FLAMES II. The Sextans dwarf spheroidal

Eline Tolstoy, Giuseppina Battaglia, José María Arroyo-Polonio +7

The Sextans dwarf spheroidal galaxy has been challenging to study in a comprehensive way as it is highly extended on the sky, with an uncertain but large tidal radius of between 80…

astro-ph.GA2023

Abundances of iron-peak elements in accreted and in situ born Galactic halo stars

P. E. Nissen, A. M. Amarsi, Á. Skúladóttir +1

Previous work on the abundances of C, O, Na, Mg, Si, Ca, Ti, Cr, Mn, Fe, Ni, Cu, and Zn in low-alpha (accreted) and high-alpha (in situ born) halo stars is extended to include the…

astro-ph.GA2023

Characterising the true descendants of the first stars

Irene Vanni, Stefania Salvadori, Ása Skúladóttir +2

The metal-poor stars in the Galactic halo are thought to show the imprints of the first (PopIII) stars, and thus provide a glance at the first episodes of star formation. In this w…

astro-ph.GA2023★ 30 cited

Tracing Pop III supernovae with extreme energies through the Sculptor dwarf spheroidal galaxy

Ása Skúladóttir, Irene Vanni, Stefania Salvadori +1

The Sculptor dwarf spheroidal galaxy is old and metal-poor, making it ideal to study the earliest chemical enrichment in the Local Group. We followed up the most metal-poor star kn…

astro-ph.GA2023★ 5 cited

Are all metal-poor stars of second-generation?

Irene Vanni, Stefania Salvadori, Ása Skúladóttir

Hydrodynamical cosmological simulations predict that the metal-free Population III (Pop III) stars were likely very massive and, therefore, short-lived. However, they left their ch…

astro-ph.GA2020★ 49 cited

Evidence for Gyr timescales of neutron star mergers from Galactic archaeology

Ása Skúladóttir, Stefania Salvadori

The nucleosynthetic site of the rapid () neutron-capture process is currently being debated. The direct detection of the neutron star merger GW170817, through gravitational wave…