21343832 A flare at BJD 2458844.77 seems to be present. 63208546 A peak at 3.375d^-1^ with a very strong harmonic suggests a 63208546 double-wave light curve with period P=0.296 d from orbital motion. 151641733 Pelisoli et al. (2020A&A...642A.180P, Cat. J/A+A/642/A180) attributed 151641733 the peak at 1.79d^-1^ as being due to rotation of the secondary. 151641733 However, there are several peaks in the range 22.7-29.7d^-1^ with 151641733 S/N between 6 and 7 which are likely g-mode pulsations. 201251043 These stars were analysed by Sahoo et al. (2020MNRAS.495.2844S) using 201251043 TESS full-frame imqages sampled with a cadence of 30 min. Although 201251043 they are listed as pulsating sdB stars, the long cadence prohibits 201251043 the detection of frequencies higher than about 24d^-1^. They all have 201251043 frequency peaks exceeding this limit. 457225725 These stars were analysed by Sahoo et al. (2020MNRAS.495.2844S) using 457225725 TESS full-frame imqages sampled with a cadence of 30 min. Although 457225725 they are listed as pulsating sdB stars, the long cadence prohibits 457225725 the detection of frequencies higher than about 24d^-1^. They all have 457225725 frequency peaks exceeding this limit. 279373920 A high-amplitude peak at 2.126d^-1^ and its harmonic indicates binary 279373920 motion with P=0.468d. 311432346 The light curve shows clear sinusoidal variations with a period 311432346 P=1.495d, which is perhaps orbital. 311898870 The main frequency peak and a marginal harmonic suggest orbital motion 311898870 with P=0.363d. 380641758 The pulsation frequencies in this star do not correspond to those 380641758 generally seen in sdB or sdO stars. Typical sdO pulsations are in the 380641758 p-mode region, which is higher than the TESS Nyquist frequency. 380641758 Perhaps they originate in the A-type companion. 421895532 A peak at 1.314d^-1^ and its harmonic indicates binary motion with 421895532 P=0.761d. The harmonic to the main peak at 6.896d^-1^ is also 421895532 present. Perhaps 0.761 d represents rotation and 0.145d the 421895532 orbital motion. 466277784 The strongest peak at 1.667d^-1^ and its harmonic suggests binary 466277784 motion with period P=0.599d. 23838673 A forest of frequencies below 10d^-1^ indicate a main sequence 23838673 {beta} Cep. There is a cut-off frequency limit for sdBV pulsation 23838673 mode excitation (about 5d^-1%) below which we do not see any 23838673 pulsation due to energy dispersion in the driving zone. However, in 23838673 this star there are some higher frequency modes of low amplitudes 23838673 visible in the periodogram, and we left it for further 23838673 investigations. 56541907 The presence of a strong peak at 7.770d^-1^ and its harmonic suggest 56541907 a binary with period P=0.129d. 124802885 TIC 124802885 (HD 154137) and TIC 301776333 (HD 289333). While both 124802885 are classified as normal main sequence stars, their luminosities are 124802885 well within the hot subdwarf range. They are not listed as subdwarf 124802885 candidates in the literature. It is possible that the Gaia parallaxes 124802885 are in error. 301776333 TIC 124802885 (HD 154137) and TIC 301776333 (HD 289333). While both 301776333 are classified as normal main sequence stars, their luminosities are 301776333 well within the hot subdwarf range. They are not listed as subdwarf 301776333 candidates in the literature. It is possible that the Gaia parallaxes 301776333 are in error. 176089274 The peak at 5.608d^-1^ has a weak harmonic suggesting orbital motion 176089274 with P=0.178d. 219641382 The light curve shows a clear sinusoidal variation with P=2.7d. 224284872 This high-lattitude faint star is listed as a candidate hot subdwarf 224284872 in Geier et al. (2019A&A...621A..38G, Cat. J/A+A/621/A38) and also in 224284872 Gontcharov et al. (2011MNRAS.413.1581G, Cat. J/MNRAS/413/1581). The 224284872 luminosity is certainly compatible with a subdwarf (no reliable 224284872 effective temperature has been measured). However, it was given an A0 224284872 classification by Slettebak & Brundage (1971AJ.....76..338S and 224284872 listed as a high-frequency A-type main sequence pulsator by 224284872 Holdsworth et al. (2014MNRAS.439.2078H, Cat. J/MNRAS/439/2078). 224284872 On the basis of the low luminosity it is a likely V1093 Her star with 224284872 a rich frequency spectrum in the range 50-130d^-1^. There are 224284872 several interesting relationships between frequencies that suggest 224284872 tidal interaction in a binary system. The presence of a peak at 224284872 0.734d^-1^ and its high-amplitude harmonic can be seen as a 224284872 double-wave variation in the light curve. This could be a result of 224284872 binary motion with period P=1.362d. The star might turn out to be a 224284872 main sequence star with incorrect parallax, but it certainly 224284872 deserves attention. 262753627 The star was also analysed by Sahoo et al. (2020MNRAS.495.2844S) using 262753627 TESS full-frame images sampled with a cadence of 30 min. It is not 262753627 listed in Van Grootel et al. (2021A&A...650A.205V, 262753627 Cat. J/A+A/650/A205). 282810113 While the single peak at 13.001d^-1^ is present, there are four other 282810113 peaks with 4