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researcher

M. Marconi

210 papers hereh-index 5116.1k citations415 works total

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

author position
  • sole author1
  • first author17
  • middle author143
  • last author26

Across the 187 of 210 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR77
  • astro-ph72
  • astro-ph.GA48
  • astro-ph.IM7
  • astro-ph.CO6
same name
  • M. Marconi — 66 papers, h 24
  • M. Marconi — 30 papers, h 8
  • M. Marconi — 21 papers, h 12
  • M. Marconi — 15 papers, h 12
  • M. Marconi — 15 papers, h 4
  • M. Marconi — 7 papers, h 2

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
19952023
most citedGaia Data Release 2: Photometric content and validation

756 citations · 8.8k across the 210 of their papers we have counts for

collaborators
Showing 2002Show all

4 papers · 1 filter

astro-ph2002★ 2 cited

Variable stars in Stellar Systems

Giuseppe Bono, Silvia Petroni, Marcella Marconi

We discuss in detail the pulsation properties of variable stars in globular clusters (GCs) and in Local Group (LG) dwarf galaxies. Data available in the literature strongly support…

astro-ph2002★ 16 cited

Anomalous RR Lyrae stars(?). III. CM Leonis

L. Di Fabrizio, G. Clementini, M. Marconi +8

Time series of B,V,I CCD photometry and radial velocity measurements from high resolution spectroscopy (R=30,000) covering the full pulsation cycle are presented for the field RR L…

astro-ph2002★ 47 cited

On the distance of Magellanic Clouds: first overtone Cepheids

G. Bono, M. A. T. Groenewegen, M. Marconi +1

We present a detailed comparison between predicted and empirical PL_{I,K} relations and Wesenheit function for Galactic and Magellanic Clouds (MCs) First Overtone (FO) Cepheids. We…

astro-ph2002★ 80 cited

Theoretical models for Bump Cepheids

G. Bono, V. Castellani, M. Marconi

We present the results of a theoretical investigation aimed at testing whether full amplitude, nonlinear, convective models account for the I-band light curves of Bump Cepheids in…

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