  We present new observations with the Precision Array for Probing the Epoch of
Reionization (PAPER) with the aim of measuring the properties of foreground
emission for 21cm Epoch of Reionization experiments at 150 MHz. We focus on the
footprint of the foregrounds in cosmological Fourier space to understand which
modes of the 21cm power spectrum will most likely be compromised by foreground
emission. These observations confirm predictions that foregrounds can be
isolated to a "wedge"-like region of 2D (k-perpendicular, k-parallel)-space,
creating a window for cosmological studies at higher k-parallel values. We also
find that the emission extends past the nominal edge of this wedge due to
spectral structure in the foregrounds, with this feature most prominent on the
shortest baselines. Finally, we filter the data to retain only this "unsmooth"
emission and image specific k-parallel modes of it. The resultant images show
an excess of power at the lowest modes, but no emission can be clearly
localized to any one region of the sky. This image is highly suggestive that
the most problematic foregrounds for 21cm EoR studies will not be easily
identifiable bright sources, but rather an aggregate of fainter emission.
