Speaker
Dr
Wei Zheng
(Johns Hopkins University)
Description
From the HST/COS spectra of selected quasars at z~>3.5, we find significant flux blueward of the HeII Lyα wavelength. The absorption profile suggests large "bubbles" of ionized helium embedded in the intergalactic medium. We find that the intensity of He+ ionizing field weakens considerably at z~3, and the reionization of the intergalactic helium started around z=3.5.