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researcher

V. Casasola

41 papers hereh-index 17798 citations51 works total

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

author position
  • first author3
  • middle author32

Across the 35 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA35
  • astro-ph.IM4
  • astro-ph.CO2
same name
  • V. Casasola — 30 papers, h 16
  • V. Casasola — 24 papers, h 5
  • V. Casasola — 8 papers, h 11
  • V. Casasola — 4 papers, h 1
  • V. Casasola — 3 papers
  • V. Casasola — 3 papers, h 3

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
20102026
most citedA systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios

217 citations · 1.5k across the 41 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.GA2021★ 1 cited

The mm-to-cm SED of spiral galaxies. Synergies between NIKA2 and SRT instruments

S. Bianchi, M. Murgia, A. Melis +9

The mm-to-cm range of the Spectral Energy Distribution of spiral galaxies remains largely unexplored. Its coverage is required to disentangle the contribution of dust emission, fre…

astro-ph.GA2021★ 7 cited

Probing the spectral shape of dust emission with the DustPedia galaxy sample

Angelos Nersesian, Wouter Dobbels, Manolis E. Xilouris +10

The objective of this paper is to understand the variance of the far-infrared (FIR) spectral energy distribution (SED) of the DustPedia galaxies, and its link with the stellar and…

astro-ph.GA2021★ 118 cited

A Nearby Galaxy Perspective on Dust Evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples

Frédéric Galliano, Angelos Nersesian, Simone Bianchi +14

Methods. We have modelled a sample of ~800 nearby galaxies, spanning a wide range of metallicity, gas fraction, specific star formation rate and Hubble stage. We have derived the d…

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