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.

D'Odorico V., Cupani G., Cristiani S., Maiolino R., Molaro P., Nonino M., et al. (2011). Optical-NIR spectra of quasars close to reionization (z˜ 6). ASTRONOMISCHE NACHRICHTEN, 332, 315-319 [10.1002/asna.201111545].

Optical-NIR spectra of quasars close to reionization (z˜ 6)

CIMATTI, ANDREA;
2011

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.
2011
D'Odorico V., Cupani G., Cristiani S., Maiolino R., Molaro P., Nonino M., et al. (2011). Optical-NIR spectra of quasars close to reionization (z˜ 6). ASTRONOMISCHE NACHRICHTEN, 332, 315-319 [10.1002/asna.201111545].
D'Odorico V.; Cupani G.; Cristiani S.; Maiolino R.; Molaro P.; Nonino M.; Cimatti A.; di Serego Alighieri S.; Fiore F.; Fontana A.; Gallerani S.; Gial...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/120734
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