A number of new radio telescopes are coming on-line paving the way to the Square Kilometre Array. Their new capabilities, e.g. large field of view, broad instantaneous band and fast response, offer new possibilities for the science. I will briefly give an overview of the facilities that are becoming available. Many of them have open time and some are planning large surveys that will be made available to the entire astronomical community, providing an important legacy. I will then focus on some of the results obtained with the Low Frequency Array (LOFAR) on topics where a strong synergy with XMM is (or should be) present. In particular, I will focus on pulsars (e.g. fast switching mode pulsars) and accreting systems among the galactic objects. For the extragalactic objects, the combination radio/X-ray is key for understanding the energetics and, therefore, the impact that radio AGN have on their surroundings. I will in particular focus on results from observations of radio galaxies and clusters. Fast response to transient objects in the radio sky is also receiving a lot of attention with LOFAR (and other radio telescopes).
|Title of host publication
|XMM-Newton: The Next Decade, Proceedings of the Conference held 9-11 May, 2016 at ESAC, Madrid
|Number of pages
|Published - 2016