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researcher

M. Bernardi

122 papers hereh-index 6227.1k citations184 works total

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

author position
  • sole author1
  • first author19
  • middle author61
  • last author10

Across the 91 of 122 papers where every author was matched, so the position is known.

fields
  • astro-ph53
  • astro-ph.GA46
  • astro-ph.CO20
  • astro-ph.IM3
same name
  • M. Bernardi — 38 papers, h 37
  • M. Bernardi — 21 papers, h 16
  • M. Bernardi — 5 papers, h 9
  • M. Bernardi — 3 papers, h 22
  • M. Bernardi — 3 papers, h 8
  • M. Bernardi — 2 papers, h 10

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
19982023
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations · 27.5k across the 122 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.CO2014★ 48 cited

On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1

Francesco Shankar, Hong Guo, Vincent Bouillot +20

The stellar mass-halo mass relation is a key constraint in all semi-analytic, numerical, and semi-empirical models of galaxy formation and evolution. However, its exact shape and r…

astro-ph.GA2014★ 200 cited

A catalogue of 2D photometric decompositions in the SDSS-DR7 spectroscopic main galaxy sample: preferred models and systematics

Alan Meert, Vinu Vikram, Mariangela Bernardi

We present a catalogue of two-dimensional, point spread function-corrected de Vacouleurs, Sérsic, de Vacouleurs+Exponential, and Sérsic+Exponential fits of ∼7×105 spectr…

astro-ph.CO2014★ 82 cited

Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe

Francesco Shankar, Simona Mei, Marc Huertas-Company +9

We compare state-of-the-art semi-analytic models of galaxy formation as well as advanced sub-halo abundance matching models with a large sample of early-type galaxies from SDSS at…

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