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M. Rossi

2 papers hereh-index 570 citations6 works total

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

author position
  • first author2

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
same name
  • M. Rossi — 19 papers, h 19
  • M. Rossi — 19 papers, h 30
  • M. Rossi — 18 papers
  • M. Rossi — 18 papers, h 11
  • M. Rossi — 16 papers, h 20
  • M. Rossi — 16 papers, h 23

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

most citedUltra-faint dwarf galaxies: unveiling the minimum mass of the first stars

54 citations · 54 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2024

Hidden Population III Descendants in Ultra-Faint Dwarf Galaxies

Martina Rossi, Stefania Salvadori, Ása Skúladóttir +2

The elusive properties of the first (Pop III) stars can be indirectly unveiled by uncovering their true descendants. To this aim, we exploit our data-calibrated model for the best-…

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★ 24 cited

The energy distribution of the first supernovae

I. Koutsouridou, S. Salvadori, Á. Skúladóttir +3

The nature of the first Pop III stars is still a mystery and the energy distribution of the first supernovae is completely unexplored. For the first time we account simultaneously…

astro-ph.GA2021★ 54 cited

Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars

Martina Rossi, Stefania Salvadori, Ása Skúladóttir

The non-detection of zero-metallicity stars in ultra-faint dwarf galaxies (UFDs) can be used to constrain the Initial Mass Function (IMF) of the first (PopIII) stars by means of a…

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