Papers
2
Total Citations
61
H-Index
2
About
M. Trifoglio is a key figure in high-energy astrophysics and instrumentation, best known for his work on gamma-ray blazars and the development of advanced monitoring systems for the Cherenkov Telescope Array (CTA). His research focuses on the multiwavelength behavior of active galactic nuclei, particularly the extreme flaring events of blazars like 3C 454.3. Trifoglio’s most cited paper, from 2010, documents the unprecedented December 2009 gamma-ray flare of 3C 454.3, when it became the brightest gamma-ray source in the sky, reaching a peak flux of ~2000 × 10⁻⁸ photons cm⁻² s⁻¹. This work, with 58 citations, was part of an intensive multifrequency campaign that provided critical insights into the physics of relativistic jets. Additionally, Trifoglio contributed to the ASTRI SST-2M prototype, a robotic telescope on Mount Etna proposed for CTA’s Small Size class. He designed the ACS/OPC-UA-based ICT infrastructure monitoring system, ensuring the telescope’s operational reliability during its scientific verification phase. His blend of observational discovery and technical innovation underscores his impact on both the study of cosmic transients and the next generation of ground-based gamma-ray observatories.
Research Focus
Key Achievements
Top Papers
- 1THE 2009 DECEMBER GAMMA-RAY FLARE OF 3C 454.3: THE MULTIFREQUENCY CAMPAIGN58 citations · 2010
- 2