  We present our results on the continuation of our survey searching for new ZZ
Ceti stars, inspired by the recently launched TESS space mission. The seven
targets were bright DA-type white dwarfs located close to the empirical ZZ Ceti
instability strip. We successfully identified one new pulsator candidate,
namely PM J22299+3024, derived detection limits for possible pulsations of four
objects for the first time, and determined new detection limits for two
targets.
