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D. Silva

6 papers hereh-index 4119 citations9 works total

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

author position
  • first author1
  • middle author3
  • last author1

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • D. Silva — 3 papers, h 3
  • D. Silva — 3 papers, h 1
  • D. Silva — 1 paper, h 0
  • D. Silva — 1 paper, h 2
  • D. Silva — 1 paper, h 3
  • D. Silva — 1 paper, h 1

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
20242026
collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

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.GA2025

That's so Retro: The Gaia-Sausage-Enceladus Merger Trajectory as the Origin of the Chemical Abundance Bimodality in the Milky Way Disk

James W. Johnson, Diane K. Feuillet, Ana Bonaca +1

The Milky Way (MW) is thought to have experienced a ∼3:1 mass-ratio merger event near redshift z∼2 with a significantly retrograde trajectory. This now-disrupted dwarf ga…

astro-ph.GA2024

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

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…

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