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researcher

M. Girardi

73 papers hereh-index 373.8k citations145 works total

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

author position
  • first author11
  • middle author43
  • last author8

Across the 62 of 73 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO33
  • astro-ph30
  • astro-ph.GA7
  • astro-ph.IM2
  • astro-ph.HE1
same name
  • M. Girardi — 39 papers, h 21
  • M. Girardi — 9 papers, h 12
  • M. Girardi — 8 papers, h 15
  • M. Girardi — 8 papers, h 2
  • M. Girardi — 6 papers, h 8
  • M. Girardi — 2 papers

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
19932026
most citedOptical Mass Estimates of Galaxy Clusters

390 citations · 3.8k across the 73 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.CO2021★ 4 cited

Accretion processes in the galaxy cluster Hydra A/Abell 780

M. Girardi, W. Boschin, M. Nonino +2

Clusters of galaxies evolve and accrete mass, mostly from small galaxy systems. Our aim is to study the velocity field of the galaxy cluster Abell 780, which is known for the power…

astro-ph.GA2021★ 47 cited

CLASH-VLT: Abell~S1063. Cluster assembly history and spectroscopic catalogue

A. Mercurio, P. Rosati, A. Biviano +31

Using the CLASH-VLT survey, we assembled an unprecedented sample of 1234 spectroscopically confirmed members in Abell~S1063, finding a dynamically complex structure at z_cl=0.3457…

astro-ph.GA2021★ 13 cited

Fossil group origins. XI. The dependence of galaxy orbits on the magnitude gap

Stefano Zarattini, Andrea Biviano, J. Alfonso L. Aguerri +2

We aim to study how the orbits of galaxies in clusters depend on the prominence of the corresponding central galaxies. We divided our data set of ∼ 100 clusters and groups int…

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