Optical-NIR spectra of quasars close to reionization (z~ 6)
V. D'Odorico, G. Cupani, S. Cristiani, R. Maiolino, P. Molaro, M., Nonino, A. Cimatti, S. di Serego Alighieri, F. Fiore, A. Fontana, S., Gallerani, E. Giallongo, F. Mannucci, A. Marconi, L. Pentericci, M. Viel, and, G. Vladilo

TL;DR
This paper presents high-quality optical-NIR spectra of three quasars near the reionization epoch (z~6), enabling insights into early universe processes like re-ionization and galaxy evolution.
Contribution
It provides new spectra of z~6 quasars and updates the cosmic mass density of C IV ions, enhancing understanding of early universe ionization history.
Findings
Confirmed constant trend of C IV cosmic mass density between redshifts 2.5 and 5.
Provided high-resolution spectra of three quasars at z~6.
Supported studies of re-ionization and early galaxy evolution.
Abstract
X-shooter, with its characteristics of resolution, spectral coverage and efficiency, provides a unique opportunity to obtain spectra of the highest-redshift quasars (z ~ 6) that will allow us to carry out successful investigations on key cosmological issues, from the details of the re-ionization process, to the evolution of the first galaxies and AGNs. In this paper, we present the spectra of three z ~ 6 quasars: one obtained during the commissioning of X-shooter and two in the context of our ongoing GTO programme. Combining this sample with data in the literature, we update the value of the C IV cosmic mass density in the range 4.5 < z < 5, confirming the constant trend with redshift between 2.5 and 5.
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