  The Green Bank North Celestial Cap (GBNCC) pulsar survey will cover the
entire northern sky ($\delta > -40^\circ$) at 350 MHz, and is one of the most
uniform and sensitive all-sky pulsar surveys to date. We have created a
pipeline to re-analyze GBNCC survey data to take a 350MHz census of all pulsars
detected by the survey, regardless of their discovery survey. Of the 1413
pulsars in the survey region, we were able to recover 661. For these we present
measured signal-to-noise ratios (S/N), flux densities, pulse widths, profiles,
and where appropriate, refined dispersion measurements (647 out of 661) and new
or improved spectral indices (276 out of 661 total, 15 new, 261 improved).
Detection scans for several hundred sources were reanalyzed in order to inspect
pulsars' single pulse behavior and 223 were confirmed to exhibit evidence of
nulling. With a detailed analysis of measured and expected S/N values and the
evolving radio frequency interference environment at 350MHz, we assess the
GBNCC survey's sensitivity as a function of spin period, dispersion measure,
and sky position. We find the sky-averaged limiting flux density of the survey
to be 0.74mJy. Combining this analysis with PsrPopPy pulsar population
simulations, we predict 60/5 non-recycled/millisecond pulsar discoveries in the
survey's remaining 21,000 pointings, and we begin to place constraints on
population model parameters.
