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C. Vignali

4 papers hereh-index 6717.6k citations610 works total

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

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • C. Vignali — 14 papers, h 3
  • C. Vignali — 14 papers, h 3
  • C. Vignali — 11 papers, h 4
  • C. Vignali — 7 papers, h 5
  • C. Vignali — 2 papers, h 1
  • C. Vignali — 1 paper, h 0

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

collaborators

4 papers

astro-ph.GA2025

Narrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis

Giovanni Mazzolari, Jan Scholtz, Roberto Maiolino +11

In this work, we spectroscopically select narrow-line AGNs (NLAGNs) among the ~300 publicly available medium-resolution spectra of the Cosmic Evolution Early Release Science Survey…

astro-ph.GA2025

The Dual Nature of GHZ9: Coexisting Active Galactic Nuclei and Star Formation Activity in a Remote X-ray Source at z = 10.145

Lorenzo Napolitano, Marco Castellano, Laura Pentericci +33

We present James Webb Space Telescope (JWST)/NIRSpec PRISM spectroscopic characterization of GHZ9 at z= 10.145 ± 0.010, currently the most distant source detected by the Chandr…

astro-ph.GA2025

JWST-discovered AGN: evidence for heavy obscuration in the type-2 sample from the first stacked X-ray detection

Andrea Comastri, Giorgio Lanzuisi, Fabio Vito +9

One of the most puzzling properties of the high-redshift AGN population recently discovered by JWST, including both broad-line and narrow-line sources, is their X-ray weakness. Wit…

astro-ph.GA2025

Intervening nuclear obscuration changing the X-ray look of the z≈6 QSO CFHQS J164121+375520

Fabio Vito, William Nielsen Brandt, Andrea Comastri +16

X-ray observations of the optically selected z=6.025 QSO CFHQS J164121+375520 (hereafter J1641) revealed that its flux dropped by a factor ≳7 from 2018, when it was a bri…

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