Armand Ciccarelli

Papers

1

Total Citations

7

H-Index

1

About

Armand Ciccarelli is an emerging astrophysicist whose research centers on the observational characterization of core-collapse supernovae, with a particular focus on their early-time photometric evolution and subtype classification. His most cited work investigates SN 2023ixf, a nearby Type II supernova, through a comprehensive multiband photometric campaign. Ciccarelli coordinated observations from nine different observatories—including the MicroObservatory network—to capture the supernova’s light curve across standard Johnson-Cousins (B, V, Rc) and Sloan (r, g) filters, as well as non-standard R, G, B, and Clear filters. His analysis suggests that SN 2023ixf may belong to the rare II-L (linear) subtype, a finding that challenges conventional classification schemes and provides critical data for understanding the diversity of massive star explosions. With 7 citations since its 2023 publication, this work has already attracted attention for its rapid-response, multi-site observational strategy. Ciccarelli’s contributions demonstrate the power of coordinated amateur-professional networks in time-domain astronomy, and his ongoing research promises to refine our models of stellar death and nucleosynthesis.

Research Focus

Key Achievements

1
H-Index
1
Papers
7
Total Citations
7
Avg Citations/Paper
🏆 Most Cited Paper
Multiband Photometry Evolution in the First Weeks of SN 2023ixf, a possible II-L Subtype Supernova
7 citations · 2023
📈 Most Prolific Year: 2023 (1 Papers)
🤝 Key Collaborators: 10

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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