The physics of the intergalactic medium
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...Theoretical studies [44, 45] suggest our universe may have had a complex star formation history: this signature of the extended ionization history is traced by the E-mode polarization power spectrum on angular scales θ > 20◦....
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...It would be more typical of the intergalactic medium (121)....
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"The physics of the intergalactic me..." refers background in this paper
...A substantial effort was made to measure PF(k) from the spectra of high redshift quasars discovered by the Sloan Digital Sky Survey (McDonald et al., 2006)....
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...The fourth occurred in 2000 with the introduction of the UV and Visible Echelle Spectrograph (UVES) to the Very Large Telescope (VLT) (D’Odorico et al., 2000), the launch of the Far Ultraviolet Spectroscopic Explorer (FUSE) (Moos et al., 2000), and the beginning of operations of the Sloan Digital Sky Survey (York et al., 2000)....
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...…the introduction of the UV and Visible Echelle Spectrograph (UVES) to the Very Large Telescope (VLT) (D’Odorico et al., 2000), the launch of the Far Ultraviolet Spectroscopic Explorer (FUSE) (Moos et al., 2000), and the beginning of operations of the Sloan Digital Sky Survey (York et al., 2000)....
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...The QSO spectra measured as part of the Sloan Digital Sky Survey (SDSS) 8 show a rapid rise in the flux decrement at z >∼ 5.5, suggesting that the epoch of H I reionization may lie not far beyond z ≃ 6....
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