  Intermediate-frequency-peaked BL Lacertae objects (IBLs) are a class of
blazars characterized by a spectral energy distribution (SED) with a
lower-energy synchrotron peak than the majority of extragalactic sources
detected by ground-based imaging atmospheric Cherenkov telescopes (IACTs).
Consequently, the peak gamma-ray flux falls outside the very-high-energy regime
(VHE, >100 GeV) covered by IACTs such as VERITAS, making IBLs difficult to
detect except during infrequent episodes of elevated flux. However, the study
of these sources in a low-flux state is essential for developing a complete
understanding of the blazar paradigm. We present the results of VHE analyses of
long-term low-flux-state observations completed for two IBL sources: 3C 66A and
W Comae. For both sources, data from VERITAS were analyzed for the VHE regime.
The study of 3C 66A extends from 2007 to 2015, resulting in a 12 standard
deviation ($\sigma$) detection from $\sim$61 observing hours. Analysis of W
Comae from 2010 to 2014, totaling $\sim$39 hours, resulted in a 6$\sigma$
low-flux-state detection. We report on the results from these VHE analyses and
describe contemporaneous multiwavelength data to be used in further analyses.
We comment on how these low-flux-state IBL detections fit within the context of
the blazar paradigm.
