so the lower mass cut is well-matched to the GOODS-S and GOODS-N samples. We separate our galaxies into local density (M$_{\mathrm{sph}}$) bins as defined in Section \[sec:localdensity\].

We then plot $<$SFR$>$ as in E07, first calculating the average SFR ($<$SFR$>$) in each r$=$1 $h^{-1}$ Mpc sphere, then binning the spheres by local density (M$_{\mathrm{sph}}$) so that each bin has at least 100 spheres in each simulation output, and finally finding the median $<$SFR$>$ in each local density bin. Results are shown as blue $\bigcirc$ ($z$=0 low resolution (LR)), orange $\bigtriangleup$ ($z$=1 LR), and red $\nabla$ ($z$=1 high resolution (HR)) in Figure \[fig-elbaz\]. The horizontal bars denote the M$_{\mathrm{sph}}$ bin sizes. The shaded regions enclose the 25th to the 75th percentiles of the $z$=1 HR (red) and $z$=0 LR (blue) samples, denoting the (lower and upper) limits of the upper and lower quartiles of the data.

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We find that in the $z$=1 HR output, the $<$SFR$>$ increases with increasing local density from M$_{\mathrm{sph}}$$\sim$5$\times$10$^{11}$ M$_{\odot}$ to M$_{\mathrm{sph}}$$\sim$10$^{13}$ M$_{\odot}$, then decreases towards the highest M$_{\mathrm{sph}}$. In the $z$=1 LR output, the $<$SFR$>$ increases up to the highest M$_{\mathrm{sph}}$. At $z$=0 the $<$SFR$>$-density relation is nearly flat until the highest M$_{\mathrm{sph}}$ bin, at 