  We present the discovery of 7 new planets and 8 planet candidates around
subgiant stars, as additions to the known sample of planets around "retired A
stars" (Johnson et al. 2006). Among these are the possible first 3-planet
systems around subgiant stars, HD 163607 and HD 4917. Additionally, we present
calculations of possible transit times, durations, depths, and probabilities
for all known planets around subgiant (3 < log g < 4) stars, focused on
possible transits during the TESS mission. While most have transit
probabilities of 1-2%, we find that there are 3 planets with transit
probabilities > 9%.
