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researcher

M. Zennaro

33 papers hereh-index 201.1k citations37 works total

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

author position
  • first author7
  • middle author13
  • last author10

Across the 30 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO30
  • astro-ph.GA1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • M. Zennaro — 8 papers, h 5
  • M. Zennaro — 6 papers, h 32
  • M. Zennaro — 2 papers, h 2
  • M. Zennaro — 2 papers, h 6
  • M. Zennaro — 2 papers, h 28
  • M. Zennaro — 1 paper, h 50

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
20162026
most citedThe BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology

199 citations · 1.4k across the 33 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.CO2019★ 98 cited

Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics

Giovanni Aricò, Raul E. Angulo, Carlos Hernández-Monteagudo +4

We present and test a framework that models the three-dimensional distribution of mass in the Universe as a function of cosmological and astrophysical parameters. Our approach comb…

astro-ph.CO2019★ 50 cited

How to add massive neutrinos to your ΛCDM simulation -- extending cosmology rescaling algorithms

Matteo Zennaro, Raúl E. Angulo, Giovanni Aricò +2

Providing accurate predictions for the spatial distribution of matter and luminous tracers in the presence of massive neutrinos is an important task, given the imminent arrival of…

astro-ph.SR2019★ 44 cited

Four stellar populations and extreme helium variation in the massive outer-halo globular cluster NGC 2419

M. Zennaro, A. P. Milone, A. F. Marino +3

Recent work revealed that both the helium variation within globular clusters (GCs) and the relative numbers of first and second-generation stars (1G, 2G) depend on the mass of the…

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