activity
20192022
most citedModeling the γ-ray Pulsar Wind Nebulae population in our Galaxy

27 citations · 120 across the 10 of their papers we have counts for

collaborators

15 papers

astro-ph.IM20224 cited

First measurements and upgrade plans of the MAGIC intensity interferometer

Juan Cortina, V. A. Acciari, A. Biland +22

The two MAGIC 17-m diameter Imaging Atmospheric Cherenkov Telescopes have been equipped to work also as an intensity interferometer with a deadtime-free, 4-channel, GPU-based, real…

astro-ph.IM20224 cited

Investigating the accuracy achievable in reconstructing the angular sizes of stars through stellar intensity interferometry observations

Michele Fiori, Giampiero Naletto, Luca Zampieri +2

Context: In recent years, stellar intensity interferometry has seen renewed interest from the astronomical community because it can be efficiently applied to Cherenkov telescope ar…

astro-ph.HE20224 cited

Deep upper limit on the optical emission during a hard X-ray burst from the magnetar SGR J1935+2154

Luca Zampieri, Sandro Mereghetti, Roberto Turolla +9

In September 2021 the magnetar SGR J1935+2154 entered a stage of burst/flaring activity in the hard X-ray band. On September 10, 2021 we observed SGR J1935+2154 with the fiber-fed…

astro-ph.HE202227 cited

Modeling the γ-ray Pulsar Wind Nebulae population in our Galaxy

M. Fiori, B. Olmi, E. Amato +4

Pulsar wind nebulae (PWNe) represent the largest class of sources that upcoming γ-ray surveys will detect. Therefore, accurate modelling of their global emission properties is one…

astro-ph.IM20219 cited

Survey of the Galactic Plane with the CherenkovTelescope Array

Q. Remy, L. Tibaldo, F. Acero +4

Observations with the current generation of very-high-energy gamma-ray telescopes have revealed an astonishing variety of particle accelerators in the Milky Way, such as supernova…

astro-ph.IM202117 cited

Stellar intensity interferometry of Vega in photon counting mode

Luca Zampieri, Giampiero Naletto, Aleksandr Burtovoi +2

Stellar Intensity Interferometry is a technique based on the measurement of the second order spatial correlation of the light emitted from a star. The physical information provided…