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Eclipsing systems are essential objects for understanding the properties ofstars and stellar systems. Eclipsing systems with pulsating components arefurthermore advantageous because they provide accurate constraints on thecomponent properties, as well as a complementary method for pulsation modedetermination, crucial for precise asteroseismology. The outcome of spacemissions aiming at delivering high-accuracy light curves for many thousands ofstars in search of planetary systems has also generated new insights in thefield of variable stars and revived the interest of binary systems in general.The detection of eclipsing systems with pulsating components has particularlybenefitted from this, and progress in this field is growing fast. In thisreview, we showcase some of the recent results obtained from studies ofeclipsing systems with pulsating components based on data acquired by the spacemissions {\it Kepler} or TESS. We consider different system configurationsincluding semi-detached eclipsing binaries in (near-)circular orbits, a(near-)circular and non-synchronized eclipsing binary with a chemicallypeculiar component, eclipsing binaries showing the heartbeat phenomenon, aswell as detached, eccentric double-lined systems. All display one or morepulsating component(s). Among the great variety of known classes of pulsatingstars, we discuss unevolved or slightly evolved pulsators of spectral type B, Aor F and red giants with solar-like oscillations. Some systems exhibitadditional phenomena such as tidal effects, angular momentum transfer,(occasional) mass transfer between the components and/or magnetic activity. Howthese phenomena and the orbital changes affect the different types ofpulsations excited in one or more components, offers a new window ofopportunity to better understand the physics of pulsations.

Eclipsing Systems with Pulsating Components (Types {\beta} Cep, {\delta} Sct, {\gamma} Dor or Red Giant) in the Era of High-Accuracy Space Data