Measuring the density of the intergalactic medium using quasar sightlines in the epoch of reionization is challenging due to the saturation of Lyman-α absorption.
Near a luminous quasar, however, the enhanced radiation creates a proximity zone observable in the quasar spectra where the Lyman-α absorption is not saturated.
In this study, we use 10 high-resolution (R ~ 10,000) z\(\sim\) 6 quasar spectra from the extended XQR-30 sample to measure the density field in the quasar proximity zones for the first time.
We find a variety of environments within 3 pMpc distance from the quasars.
Introduction: Quasar Proximity Zones
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