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The bRing robotic observatory network was built to search for circumplanetarymaterial within the transiting Hill sphere of the exoplanet $\beta$ Pic bacross its bright host star $\beta$ Pic. During the bRing survey of $\beta$Pic, it simultaneously monitored the brightnesses of thousands of bright starsin the southern sky ($V$ $\simeq$ 4-8, $\delta$ $\lesssim$ -30$^{\circ}$). Inthis work, we announce the discovery of $\delta$ Scuti pulsations in the A-typestar HD 156623 using bRing data. HD 156623 is notable as it is a well-studiedyoung star with a dusty and gas-rich debris disk, previously detected usingALMA. We present the observational results on the pulsation periods andamplitudes for HD 156623, discuss its evolutionary status, and provide furtherconstraints on its nature and age. We find strong evidence of frequencyregularity and grouping. We do not find evidence of frequency, amplitude, orphase modulation for any of the frequencies over the course of theobservations. We show that HD 156623 is consistent with other hot and highfrequency pre-MS and early ZAMS $\delta$ Scutis as predicted by theoreticalmodels and corresponding evolutionary tracks, although we observe that HD156623 lies hotter than the theoretical blue edge of the classical instabilitystrip. This, coupled with our characterization and Sco-Cen membership analyses,suggest that the star is most likely an outlying ZAMS member of the $\sim$16Myr Upper Centaurus-Lupus subgroup of the Sco-Cen association.

Discovery of {\delta} Scuti Pulsations in the Young Hybrid Debris Disk Star HD 156623