  The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep
Extragalactic Legacy Survey Fields (UVCANDELS) program provides HST/UVIS F275W
imaging for four CANDELS fields. We combine this UV imaging with existing
HST/near-IR grism spectroscopy from 3D-HST$+$AGHAST to directly compare the
resolved rest-frame UV and H$\alpha$ emission for a sample of 979 galaxies at
$0.7<z<1.5$ spanning a range in stellar mass of $10^{8-11.5}$ M$_\odot$. Using
a stacking analysis, we perform a resolved comparison between homogenized maps
of rest-UV and H$\alpha$ to compute the average UV-to-H$\alpha$ luminosity
ratio (an indicator of burstiness in star-formation) as a function of
galactocentric radius. We find that galaxies below stellar mass of
$\sim$10$^{9.5}$ M$_\odot$, at all radii, have a UV-to-H$\alpha$ ratio higher
than the equilibrium value expected from constant star-formation, indicating a
significant contribution from bursty star-formation. Even for galaxies with
stellar mass $\gtrsim$10$^{9.5}$ M$_\odot$, the UV-to-H$\alpha$ ratio is
elevated towards in their outskirts ($R/R_{eff}>1.5$), suggesting that bursty
star-formation is likely prevalent in the outskirts of even the most massive
galaxies but is likely over-shadowed by their brighter cores. Furthermore, we
present the UV-to-H$\alpha$ ratio as a function of galaxy surface brightness, a
proxy for stellar mass surface density, and find that regions below
$\sim$10$^{7.5}$ M$_\odot$ kpc$^{-2}$ are consistent with bursty
star-formation, regardless of their galaxy stellar mass, potentially suggesting
that local star-formation is independent of global galaxy properties at the
smallest scales. Lastly, we find galaxies at $z>1.1$ to have bursty
star-formation regardless of radius or surface brightness.
