  This work is dedicated to a search for new pulsating hot subdwarfs in TESS
photometric data which could have been missed in previous searches. By matching
catalogues of hot subdwarfs with TESS targets and using luminosities from Gaia
parallaxes, a list of 1389 candidate hot subdwarfs observed by TESS was
created. The periodograms of these stars were inspected, and the stars were
classified according to variability type. An updated catalogue of all known
pulsating hot subdwarfs is presented. A number of probable pulsating binaries
have been identified, which might prove useful for verifying the asteroseismic
masses. The mean masses of p- and g-mode pulsators are estimated from the
stellar parameters. A list of 63 previously unknown pulsating hot subdwarfs
observed by TESS is presented. More than half of the stars previously
identified as pure p-mode pulsators are found to have frequencies in the g-mode
region as well. As a result, hybrid p- and g-mode pulsators occur over the
whole instability strip.
