activity
20152026
most citedScience with the Cherenkov Telescope Array

241 citations · 855 across the 45 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.HE2022★ 19 cited

Investigating the origin of optical and X-ray pulsations of the transitional millisecond pulsar PSR J1023+0038

G. Illiano, A. Papitto, F. Ambrosino +21

PSR J1023+0038 is the first millisecond pulsar that was ever observed as an optical and UV pulsar. So far, it is the only optical transitional millisecond pulsar. The rotation- and…

astro-ph.HE2022★ 12 cited

Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide

A. D'Aì, E. Amato, A. Burtovoi +52

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array will be composed of nine imaging atmospheric Cherenkov telescopes at the Observatorio del Teide site…

astro-ph.HE2022★ 56 cited

ASTRI Mini-Array Core Science at the Observatorio del Teide

S. Vercellone, C. Bigongiari, A. Burtovoi +84

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the Obse…

astro-ph.SR2022★ 56 cited

Observation of Magnetic Switchback in the Solar Corona

Daniele Telloni, Gary P. Zank, Marco Stangalini +49

Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mec…

astro-ph.HE2022★ 4 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.HE2022★ 27 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…