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XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch

D'odorico, V; Bañados, E; Becker, GD; Bischetti, M; Bosman, SEI; Cupani, G; Davies, R; ... Zanchettin, MV; + view all (2023) XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch. Monthly Notices of the Royal Astronomical Society , 523 (1) pp. 1399-1420. 10.1093/mnras/stad1468. Green open access

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Abstract

The final phase of the reionization process can be probed by rest-frame UV absorption spectra of quasars at z ≳ 6, shedding light on the properties of the diffuse intergalactic medium within the first Gyr of the Universe. The ESO Large Programme 'XQR-30: the ultimate XSHOOTER legacy survey of quasars at z ≃ 5.8-6.6' dedicated ∼250 h of observations at the VLT to create a homogeneous and high-quality sample of spectra of 30 luminous quasars at z ∼6, covering the rest wavelength range from the Lyman limit to beyond the Mg ii emission. Twelve quasar spectra of similar quality from the XSHOOTER archive were added to form the enlarged XQR-30 sample, corresponding to a total of ∼350 h of on-source exposure time. The median effective resolving power of the 42 spectra is R ≃ 11 400 and 9800 in the VIS and NIR arm, respectively. The signal-to-noise ratio per 10 km s-1 pixel ranges from ∼11 to 114 at λ ≃ 1285 Å rest frame, with a median value of ∼29. We describe the observations, data reduction, and analysis of the spectra, together with some first results based on the E-XQR-30 sample. New photometry in the H and K bands are provided for the XQR-30 quasars, together with composite spectra whose characteristics reflect the large absolute magnitudes of the sample. The composite and the reduced spectra are released to the community through a public repository, and will enable a range of studies addressing outstanding questions regarding the first Gyr of the Universe.

Type: Article
Title: XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stad1468
Publisher version: https://doi.org/10.1093/mnras/stad1468
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. - For the purpose of open access, the authors have applied a Creative Commons Attribution (CC BY) licence to any Author Accepted Manuscript version arising from this submission.
Keywords: galaxies: high-redshift; intergalactic medium; quasars: absorption lines; quasars: emission lines; dark ages; reionization; first stars
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10173151
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