Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z~6
arXiv:2009.06648 · doi:10.3847/1538-4357/abb80b
Abstract
We present measurements of the size of the quasar proximity zone () for eleven low-luminosity () quasars at , discovered by the Subaru High- Exploration of Low-Luminosity Quasars project (SHELLQs). Our faint quasar sample expands the measurement down to mag, where more common quasar populations dominate at the epoch. We restrict the sample to quasars whose systemic redshifts have been precisely measured by [CII] 158 m or MgII 2798 emission lines. We also update the measurements for 26 luminous quasars presented in Eilers et al. (2017)(arXiv:1703.02539) by using the latest systemic redshift results. The luminosity dependence on is found to be consistent with the theoretical prediction assuming highly ionized intergalactic medium. We find a shallow redshift evolution of the luminosity-corrected , () over . This trend is steeper than that of Eilers et al. (2017) but significantly shallower than those of the earlier studies. Our results suggest that is insensitive to the neutral fraction of the universe at . Four quasars show exceptionally small ( proper Mpc), which could be the result of their young age ( yr) in the reionization epoch, though statistics is still small.
arXiv comment14 pages, 8 figures, Accepted for publication in ApJ
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