  The Solar Aspect Monitor (SAM) is a pinhole camera on the Extreme-ultraviolet
Variability Experiment (EVE) aboard the Solar Dynamics Observatory (SDO). SAM
projects the solar disk onto the CCD through a metallic filter designed to
allow only solar photons shortward of 7 nm to pass. Contamination from
energetic particles and out-of-band irradiance is, however, significant in the
SAM observations. We present a technique for isolating the 0.01--7 nm
integrated irradiance from the SAM signal to produce the first results of
broadband irradiance for the time period from May 2010 to May 2014. The results
of this analysis agree with a similar data product from EVE's EUV
SpectroPhotometer (ESP) to within 25%. We compare our results with measurements
from the Student Nitric Oxide Explorer (SNOE) Solar X-ray Photometer (SXP) and
the Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) Solar
EUV Experiment (SEE) at similar levels of solar activity. We show that the
full-disk SAM broadband results compare well to the other measurements of the
0.01--7 nm irradiance. We also explore SAM's capability toward resolving
spatial contribution from regions of solar disk in irradiance and demonstrate
this feature with a case study of several strong flares that erupted from
active regions on March 11, 2011.
