  Blazars are the most abundant type of extragalactic gamma-ray source, usually
presenting high variability across the electromagnetic spectrum. Their Very
High Energy (VHE, above 0.1 TeV) emission has been studied in detail using Air
Cherenkov Telescopes, with observations biased to flaring periods while their
average activity has not been properly characterized. In this work, we report
the results of 2090 days of quasi-continuous observations of the blazars 1ES
1215+303 and VER J0521+211, carried out with the High Altitude Water Cherenkov
(HAWC) gamma-ray observatory. Fitting a power-law attenuated by photon-photon
interaction with the extragalactic background light, we obtained a 6.2 $\sigma$
level detection for 1ES 1215+303 and a 4.3 $\sigma$ marginal detection for VER
J0521+211. With the inclusion of the HAWC TeV spectrum, we built
quasi-simultaneous multiwavelength spectral distributions and fitted a leptonic
emission model to the observed data.
