Location of the spectroscopically identified pulsating sdB stars in the T_eff−log g plane. Known pulsating sdBs, collected from Uzundag et al. (2024) and Baran et al. (2024), are shown as blue dots. Newly discovered pulsating sdBs, for which atmospheric parameters are known (Table 2), are represented by solid red squares. Open symbols indicate variables from the ‘binary candidates’ and ‘low relativelikelihood pulsators/binary candidates’ groups. Evolutionary models from Uzundag et al. (2021) for M_ZAHB = 0.467, 0.4675, 0.468, 0.4685, and 0.47 M_☉ are shown in green.