  We report on the detection of seven bursts from the periodically active,
repeating fast radio burst (FRB) source FRB 180916.J0158+65 in the 300-400-MHz
frequency range with the Green Bank Telescope (GBT). Emission in multiple
bursts is visible down to the bottom of the GBT band, suggesting that the
cutoff frequency (if it exists) for FRB emission is lower than 300 MHz.
Observations were conducted during predicted periods of activity of the source,
and had simultaneous coverage with the Low Frequency Array (LOFAR) and the FRB
backend on the Canadian Hydrogen Intensity Mapping Experiment (CHIME)
telescope. We find that one of the GBT-detected bursts has potentially
associated emission in the CHIME band (400-800 MHz) but we detect no bursts in
the LOFAR band (110-190 MHz), placing a limit of $\alpha > -1.0$ on the
spectral index of broadband emission from the source. We also find that
emission from the source is severely band-limited with burst bandwidths as low
as $\sim$40 MHz. In addition, we place the strictest constraint on observable
scattering of the source, $<$ 1.7 ms, at 350 MHz, suggesting that the
circumburst environment does not have strong scattering properties.
Additionally, knowing that the circumburst environment is optically thin to
free-free absorption at 300 MHz, we find evidence against the association of a
hyper-compact HII region or a young supernova remnant (age $<$ 50 yr) with the
source.
