{ "id": "2307.12421", "version": "v1", "published": "2023-07-23T20:22:01.000Z", "updated": "2023-07-23T20:22:01.000Z", "title": "Crossing the Rubicon of Reionization with z~5 QSOs", "authors": [ "A. Grazian", "K. Boutsia", "E. Giallongo", "S. Cristiani", "F. Fontanot", "M. Bischetti", "A. Bongiorno", "G. Calderone", "G. Cupani", "V. D'Odorico", "C. Feruglio", "F. Fiore", "F. Guarneri", "M. Porru", "I. Saccheo" ], "comment": "Accepted for publication in ApJ", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "One of the key open questions in Cosmology is the nature of the sources that completed the cosmological hydrogen Reionization at z~5.2. High-z primeval galaxies have been long considered the main drivers for Reionization, with a minor role played by high-z AGN. However, in order to confirm this scenario, it is fundamental to measure the photo-ionization rate produced by active SMBHs close to the epoch of Reionization. Given the pivotal role played by spectroscopically complete observations of high-z QSOs, in this paper we present the first results of the RUBICON (Reionizing the Universe with BrIght COsmological Nuclei) survey. It consists of a color selected sample of bona-fide z~5 QSO candidates from the Hyper Suprime-Cam Subaru Strategic Survey. Our QSO candidates have been validated both by photometric redshifts based on SED fitting and by spectroscopic redshifts, confirming that they lie at 4.5