Homogeneous measurements of proximity zone sizes for 59 quasars in the Epoch of Reionization
The overionized regions surrounding high-redshift quasars, known as proximity zones, provide a window into the interaction between supermassive black holes (SMBHs) and the intergalactic medium (IGM) during the epoch of reionization (EoR). We present new homogeneous measurements of proximity zone sizes ($R_{\mathrm{p}}$) for a sample of $59$ quasars spanning redshifts $5.77 \leq z \leq 7.54$ (median $z = 6.59$). For $15$ of these sources, we measure $R_{\mathrm{p}}$ for the first time. The quasars in our catalog have absolute magnitudes at rest-frame $1450$ Å in the range $-29.13 \leq M_{1450} \leq -25.20$ (median $M_{1450} \simeq -26.49$), providing one of the most extensive data sets for exploring $R_{\mathrm{p}}$ at these epochs. The distribution of $R_{\mathrm{p}}$ values shows a large scatter at fixed redshift and luminosity, likely reflecting variations in quasar lifetimes ($t_{\mathrm{Q}}$), IGM density fluctuations, and IGM neutral fraction. We fit a bivariate power-law model to a large sample of $100$ objects to study the dependence of $R_{\mathrm{p}}$ with both $M_{1450}$ and $z$: we find that the evolution of $R_{\mathrm{p}}$ with luminosity is in agreement with the models ($R_{\mathrm{p}} \propto 10^{-0.4 M_{1450}/2.87}$), while the evolution of $R_{\mathrm{p}}$ with $z$ is steeper than previous works ($R_{\mathrm{p}} \propto (1+z)^{-2.44}$). We identify $13$ quasars with small proximity zone size, defined using the residuals of our fit. In all cases, except for J2211$-$6320, we rule out the presence of associated dense absorbers that prematurely truncate $R_{\mathrm{p}}$, and suggest a short $t_{\mathrm{Q}}$ ($\lesssim 10^4$ yr) as a possible explanation for their small proximity zone sizes.