  The discovery of the high-frequency-peaked BL Lac object 1ES 0806+524
(z=0.138) as a source of very-high-energy (VHE, E>100 GeV) gamma-ray photons
was announced in 2008 by the VERITAS Collaboration, at a level of 1.8% of the
Crab Nebula flux above 300 GeV. Since then, VERITAS has continued observing the
source over multiple seasons, significantly improving the significance of the
detection. We report the results of the analysis of the 2006-2014 VERITAS data,
corresponding to a total exposure of about 70 hours. We present the new,
average VHE spectrum of the source, together with the multi-year light-curve
constraining long-term VHE variability.
