Radiative lifetimes and atomic transition probabilities have been meas
ured for over 35 neutral and singly ionized species in the Wisconsin A
tomic Transition Probabilities (WATP) Program since it began in 1980.
Radiative lifetimes are measured using time-resolved laser-induced flu
orescence of a slow atomic/ionic beam. These lifetimes are combined wi
th branching fractions to yield absolute atomic transition probabiliti
es for neutral and singly ionized species. The branching fractions are
determined from emission spectra recorded using the 1.0 m Fourier-tra
nsform spectrometer at the National Solar Observatory. The current foc
us of the WATP Program is on the rare-earth elements, in particular Tm
, Dy, and Po.