Abstract
I extract a small, clean sample of Lyman Alpha Emitters from z ≈ 3.0 to 3.5 from the HETDEX Data Release 1 and stack the 1D detection spectra to explore the feasibility of detecting (in ensemble) Lyman Continuum photons (880-910 Å) for future correlation with measurable characteristics of individual galaxies and ensembles of galaxies with the ultimate goal of constraining the escape of extreme UV radiation from galactic analogs during the Epoch of Reionization.