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C. Vignali

23 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
  • sole author1
  • first author8
  • middle author5
  • last author6

Across the 20 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph23
same name
  • C. Vignali — 2 papers
  • C. Vignali — 1 paper, h 24

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
19972005
most citedThe HELLAS2XMM 1dF survey: on the nature of high X-ray to optical flux ratio sources

1 citations · 1 across the 7 of their papers we have counts for

collaborators
Showing 1997Show all

4 papers · 1 filter

astro-ph1997

ASCA detection of the FeK edge in the spectrum of the Seyfert 2 galaxy IRAS 04575-7537: a sign of a complex absorber

C. Vignali, A. Comastri, G. M. Stirpe +5

ASCA X-ray spectral analysis of the Seyfert 2 galaxy IRAS 04575-7537 is presented. The main result is the presence of a significant iron edge at a rest energy of 7.13^+0.21_-0.16 k…

astro-ph1997

Highly Ionized Neon in the Spectrum of the Sey 2 Galaxy NGC 4507 ?

C. Vignali, R. Audano, A. Comastri +2

Results of an ASCA X-ray observation of NGC 4507 are presented. The spectrum is best parameterized by a double power law (or a partial covering) model plus a narrow FeKα emission…

astro-ph1997

ASCA and ROSAT X-ray Spectra of IC 5063 and NGC 3998

C. Vignali, A. Comastri, M. Cappi +1

The results of the 0.1-10 keV spectral analysis of IC 5063 (Narrow Line Radio Galaxy) and NGC 3998 (LINER) are presented. In both cases there is evidence of a FeKα emission line,…

astro-ph1997

The First High-Energy X-Ray Spectrum of a Z>2 Radio-Quiet Quasar: Q1101-264

C. Vignali, A. Comastri, M. Cappi +1

Results of the X-ray spectral analysis of the high-redshift radio-quiet quasar Q1101-264 are presented. The ASCA spectrum suggests a marginal evidence of a FeKα emission line at…

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