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researcher

G. Cescutti

23 papers hereh-index 9326 citations49 works total

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

author position
  • first author3
  • middle author14
  • last author2

Across the 19 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR9
  • astro-ph.HE5
  • nucl-ex5
  • physics.ins-det3
  • astro-ph.GA1
same name
  • G. Cescutti — 79 papers, h 26
  • G. Cescutti — 15 papers, h 7
  • G. Cescutti — 13 papers, h 4
  • G. Cescutti — 4 papers
  • G. Cescutti — 2 papers, h 1

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 citedUncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations

79 citations · 316 across the 22 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

physics.ins-det2024

Towards a new generation of solid total-energy detectors for neutron-capture time-of-flight experiments with intense neutron beams

J. Balibrea-Correa, V. Babiano-Suarez, J. Lerendegui-Marco +134

Challenging neutron-capture cross-section measurements of small cross sections and samples with a very limited number of atoms require high-flux time-of-flight facilities. In turn,…

astro-ph.SR2024★ 8 cited

A combined study of thermohaline mixing and envelope overshooting with PARSEC: Calibration to NGC 6397 and M4

C. T. Nguyen, A. Bressan, A. J. Korn +7

Thermohaline mixing is one of the main processes in low-mass red giant stars that affect the transport of chemicals and, thus, the surface abundances along the evolution. The inter…

astro-ph.GA2024★ 26 cited

(Re)mind the gap: a hiatus in star formation history unveiled by APOGEE DR17

E. Spitoni, F. Matteucci, R. Gratton +3

The analysis of several spectroscopic surveys indicates the presence of a bimodality between the disc stars in the abundance ratio space of [α/Fe] versus [Fe/H]. The two stellar…

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