“…Our understanding of the Galactic population of MSPs and, more generally, recycled pulsars over the past decade has been significantly improved. This is thanks, in large part, to a great increase in sample size provided by a number of large-scale surveys of the Galactic disk at Parkes [46], Green Bank [47], Arecibo [48], Effelsberg [49] and the Low-Frequency Array [50]. These surveys have greatly increased the sample size such that the number of Galactic MSPs now outnumbers their counterparts in globular clusters.…”