  We report the discovery of three new pulsars in the Globular Cluster (GC)
NGC6517, namely NGC 6517 E, F, and G, made with the Five-hundred-meter Aperture
Spherical radio Telescope (FAST). The spin periods of NGC 6517 E, F, and G are
7.60~ms, 24.89~ms, and 51.59~ms, respectively. Their dispersion measures are
183.29, 183.713, and 185.3~pc~cm$^{-3}$, respectively, all slightly larger than
those of the previously known pulsars in this cluster. The spin period
derivatives are at the level of 1$\times$10$^{-18}$~s~s$^{-1}$, which suggests
these are recycled pulsars. In addition to the discovery of these three new
pulsars, we updated the timing solutions of the known isolated pulsars, NGC
6517 A, C, and D. The solutions are consistent with those from Lynch et al.
(2011) and with smaller timing residuals. From the timing solution, NGC 6517 A,
B (position from Lynch et al. 2011), C, E, and F are very close to each other
on the sky and only a few arcseconds from the optical core of NGC 6517. With
currently published and unpublished discoveries, NGC6517 now has 9 pulsars,
ranking 5$^{th}$ of the GCs with the most pulsars. The discoveries take
advantage of the high sensitivity of FAST and a new algorithm used to check and
filter possible candidate signals.
