Yield of events with NS lenses detectable with Roman in photometry and astrometry over the entire GBTDS duration as a function of mean kick velocity v_kick before (dotted green) and after (solid purple) applying the effect of natal kicks on the volume density of NSs in the Galaxy. The error bars represent the Poisson noise; the ${\sigma }^2={\sum }_i{w}_i^2$ formula (Barlow 1987) is applied to the weighted Poisson counts. While stronger kicks increase the probability of lensing by a single NS, this effect is counterbalanced in weighting by a lower number of NSs that are available as lenses in the inner Galactic regions.