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C. Ventura

8 papers hereh-index 117 citations6 works total

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

author position
  • middle author6

Across the 6 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.CO2
  • astro-ph.HE2
  • astro-ph.SR1
same name
  • C. Ventura — 26 papers, h 16
  • C. Ventura — 17 papers, h 18
  • C. Ventura — 3 papers, h 1
  • C. Ventura — 3 papers, h 1
  • C. Ventura — 1 paper, h 1
  • C. Ventura — 1 paper, 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

most citedEP 250108a/SN 2025kg: Observations of the most nearby Broad-Line Type Ic Supernova following an Einstein Probe Fast X-ray Transient

1 citations · 1 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2026

The dwarf galaxy NGC 185: the flagship of Andromeda's dwarf galaxies for the study of evolved multiple stellar populations

Paolo Ventura, Chiara Ventura, Richard D'Souza +6

Reaching galaxies at 10-15 Mpc with HST and JWST requires star formation history (SFH) diagnostics that do not rely on the faint main sequence turn-off. We investigate whether hori…

astro-ph.GA2026

Globular Clusters in the Time of the JWST. I. Survey Design and First Results on Multiple Populations and Beyond

A. P. Milone, A. F. Marino, G. Cordoni +25

Globular clusters (GCs) host multiple stellar populations with distinct chemical compositions, but their properties among very low-mass stars remain poorly constrained. The James W…

astro-ph.GA2026

The applicability of the JAGB method for measuring the distance of galaxies subject to different metal enrichment rates

Claudio Gavetti, Paolo Ventura, Flavia Dell'Agli +4

The JAGB method has been proposed in recent years as a possible distance indicator for galaxies in the Local Group and beyond. However, the nature of the stars populating the J reg…

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