activity
20132026
most citedSensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

135 citations · 969 across the 51 of their papers we have counts for

collaborators
Showing 2021Show all

7 papers · 1 filter

astro-ph.HE2021★ 13 cited

A MeerKAT, e-MERLIN, H.E.S.S. and Swift search for persistent and transient emission associated with three localised FRBs

James O. Chibueze, M. Caleb, L. Spitler +156

We report on a search for persistent radio emission from the one-off Fast Radio Burst (FRB) 20190714A, as well as from two repeating FRBs, 20190711A and 20171019A, using the MeerKA…

astro-ph.HE2021★ 72 cited

The Hunt for Pevatrons: The Case of Supernova Remnants

P. Cristofari

The search for Galactic pevatrons is now a well-identified key science project of all instruments operating in the very-high-energy domain. Indeed, in this energy range, the detect…

astro-ph.HE2021★ 4 cited

Multi-messenger and transient astrophysics with the Cherenkov Telescope Array

Ž. Bošnjak, A. M. Brown, A. Carosi +142

The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics co…

astro-ph.HE2021★ 7 cited

Gamma rays and neutrinos from RX J1713.7-3946 in a lepto-hadronic scenario

Pierre Cristofari, Viviana Niro, Stefano Gabici

The gamma-ray emission of RX J1713.7-3946, despite being extensively studied in the GeV and TeV domain, remains poorly understood. This is mostly because in this range, two competi…

astro-ph.HE2021★ 34 cited

Particle acceleration and multimessenger emission from starburst-driven galactic winds

Enrico Peretti, Giovanni Morlino, Pasquale Blasi +1

The enhanced star forming activity, typical of starburst galaxies, powers strong galactic winds expanding on kiloparsec (kpc) scales and characterized by bubble structures. Here we…

astro-ph.HE2021★ 46 cited

Cosmic ray protons and electrons from supernova remnants

P. Cristofari, P. Blasi, D. Caprioli

The spectrum of cosmic ray protons and electrons released by supernova remnants throughout their evolution is poorly known, because of the difficulty in accounting for particle esc…

astro-ph.HE2021★ 128 cited

Particle acceleration in winds of star clusters

Giovanni Morlino, Pasquale Blasi, Enrico Peretti +1

The origin of cosmic rays in our Galaxy remains a subject of active debate. While supernova remnant shocks are often invoked as the sites of acceleration, it is now widely accepted…