Redshift of reionization: are we there yet?

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dc.creatorGnedin, Nickolay Y.
dc.date2001-10-12
dc.date.accessioned2026-07-07T02:00:48Z
dc.date.available2026-07-07T02:00:48Z
dc.descriptionComparison of the observed evolution of the Ly-alpha transmitted flux in the spectra of four highest redshift quasars discovered by SLOAN survey with the theoretical prediction for this evolution based on the state-of-the-art numerical simulations of cosmological reionization already allows one to constrain the redshift of reionization to z = 6.2 +- 0.1s +- 0.2r, where systematic and random errors are given respectively.
dc.descriptionSubmitted to MNRAS pink pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0110290
dc.identifierhttp://arxiv.org/abs/astro-ph/0110290
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3529
dc.subjectAstrophysics
dc.titleRedshift of reionization: are we there yet?
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