1. Constraining models of the pulsar wind nebula in SNR G0.9+0.1 via simulation of its detection properties using the Cherenkov Telescope Array. Issue 3 (2nd October 2020) Authors: Fiori, M; Zampieri, L; Burtovoi, A; Caraveo, P; Tibaldo, L Journal: Monthly notices of the Royal Astronomical Society Issue: Volume 499:Issue 3(2020) Page Start: 3494 Record Type: Journal Article View Content: Available online (eLD content is only available in our Reading Rooms) ↗