E. Nardini

Arcetri Astrophysical Observatory

Papers

1

Total Citations

23

H-Index

1

About

E. Nardini is a leading astrophysicist specializing in the study of active galactic nuclei (AGN) and supermassive black holes, with a particular focus on the complex interplay between accretion disks, coronae, and outflows. Their major contributions lie in multiwavelength reverberation mapping—using coordinated X-ray, UV, and optical observations to probe the innermost regions of AGN. A standout achievement is their work on the bright Seyfert galaxy Ark 120, where a coordinated 50-day Swift campaign and ground-based monitoring revealed critical time delays between X-ray, UV, and optical emissions. This research, published in 2020 and cited 23 times, provides direct insights into the geometry and physics of the accretion flow and corona, challenging standard models of AGN variability. Nardini’s work has significantly advanced our understanding of how black holes accrete matter and produce high-energy radiation, making them a key figure in AGN astrophysics. Their findings continue to shape observational strategies for next-generation X-ray observatories.

Research Focus

Key Achievements

1
H-Index
1
Papers
23
Total Citations
23
Avg Citations/Paper
🏆 Most Cited Paper
X-ray, UV, and optical time delays in the bright Seyfert galaxy Ark 120 with co-ordinated <i>Swift</i> and ground-based observations
23 citations · 2020
📈 Most Prolific Year: 2020 (1 Papers)
🤝 Key Collaborators: 19
🏛 Institutions: Arcetri Astrophysical Observatory

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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