  We report calculations of energy levels, radiative decay rates, and lifetimes
for transitions among the 3s$^2$3p$^5$, 3s3p$^6$, and 3s$^2$3p$^4$3d
configurations of Cl-like W LVIII. The general-purpose relativistic atomic
structure package (GRASP) has been adopted for our calculations. Comparisons
are made with the most recent results of Mohan et al. [Can. J. Phys. {\bf 92}
(2014) xxx] and discrepancies in lifetimes are noted, up to four orders of
magnitude in some instances. Our energy levels are estimated to be accurate to
better than 0.5\%, whereas results for radiative rates and lifetimes should be
accurate to better than 20\%.
