E. Bozzo

TL;DR: In this article, the ephemeris of the eclipsing high-mass X-ray binary (HMXB) systems LMC X-4, Cen X-3, 4U 1700-377, 4 U 1538-522, SMC X-1, IGR J18027-2016, Vela X 1, VELA X 1, IGRJ17252-3616, XTE J1855-026, and OAO 1657-415 with the help of more than ten years of monitoring these sources with the All

TL;DR: In this article, the first extensive radio to gamma-ray observations of a fast-rising blue optical transient (FBOT), AT2018cow, over its first ~100 days were presented.

TL;DR: In this article, the Lighthouse nebula and its jet-like X-ray structure were observed through dedicated high spatial resolution observations in X-rays (Chandra) and radio band (ATCA), and it was shown that the feature is a true pulsar's jet.

TL;DR: In this paper, the authors carried out an in-depth spectral and timing analysis of these XMM-Newton data and provided strong convincing evidence that the supergiant fast X-ray transients were produced by the accretion of matter from a massive clump onto the compact object hosted in this system.

TL;DR: In this paper, the authors summarize past electromagnetic follow-up efforts as well as the organization and policy of the current EM followup program and compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow up observations that were performed in the different bands.