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Technological spin-offs

INAF, despite its young age, already has thirty patents and can claim industrial spin-offs in sectors from ophthalmology (for the cure of cataracts for example) to medicine (orthopaedics and dentistry in particular). From art to sport, from security to the environment. The ratio of investment to economic return reaches a factor of 100 in some cases. At the last EXPO in Shanghai, amongst the Small and Medium Enterprises selected by the Italian government to represent national excellence, was Novaetech of Naples, that thanks to an INAF spin-off, has developed a balance so sensitive that it can weigh the fine dust particles that threaten the environment in our cities.

The Lucchin Schools Return

Jun 01, 2025

The Lucchin Schools Return First Edition of the New INAF PhD School Series Concludes in Asiago

MISTRAL, a wind of change in the SRT observations

May 29, 2025

MISTRAL, a wind of change in the SRT observations MISTRAL is a new-generation receiver for observations at millimeter wavelengths, built as part of the recent project to upgrade the Sardinia Radio Telescope for the study of the high-frequency radio universe. The main features of this instrument are the very high number of detectors cooled to temperatures close to absolute zero and a dedicated cold optical system, which allow for extremely sharp images. MISTRAL made its “first light” by observing three different celestial objects: the Orion Nebula, the radio lobes of the supermassive black hole in the galaxy M87, and the supernova remnant Cassiopeia A. These images represent the first scientific observations at 90 GHz ever obtained using the SRT

Unlocking the secrets of the first Quasars: how they defy the laws of Physics to grow

Nov 20, 2024

Unlocking the secrets of the first Quasars: how they defy the laws of Physics to grow New evidence has been discovered explaining how supermassive black holes formed in the first billion years of the Universe's life. The study, conducted by INAF researchers, analyses 21 distant quasars and reveals that these objects are in a phase of extremely rapid accretion. This provides valuable insights into their formation and evolution, together with that of their host galaxies