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researcher

R. Lucchesi

15 papers hereh-index 9204 citations17 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • middle author11
  • last author1

Across the 15 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA12
  • astro-ph.SR2
  • astro-ph.IM1
same name
  • R. Lucchesi — 1 paper, h 12

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20192026
most citedThe Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk

92 citations · 378 across the 15 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

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]~<−2.0) in the solar neighbourhood (within ∼2 kpc), selected to be on planar or…

astro-ph.GA2024★ 12 cited

The Pristine Inner Galaxy Survey (PIGS) X. Probing the early chemical evolution of the Sagittarius dwarf galaxy with carbon abundances

Federico Sestito, Anke Ardern-Arentsen, Sara Vitali +6

We aim to constrain the chemo-dynamical properties of the Sagittarius (Sgr) dwarf galaxy using carbon abundances. Our sample from the \textit{Pristine} Inner Galaxy Survey (PIGS) i…

astro-ph.SR2024

On the Pair-Instability Supernova origin of J1010+2358

Ása Skúladóttir, Ioanna Koutsouridou, Irene Vanni +4

The first (Pop III) stars formed only out of H and He and were likely more massive than present-day stars. Massive Pop III stars in the range 140-260 M⊙​ are predicted to end…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.