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Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts

, , , , and . (2019)cite arxiv:1909.12309Comment: 17 pages, 5 figures, 2 appendices.

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The most luminous blue quasars at 3.0<z<3.3. II. CIV/X-ray emission and accretion disc physics, , , , , , , , , and 5 other author(s). (2021)cite arxiv:2107.02806Comment: 22 pages, 15 figures (with 3 more figures in the Appendix), abstract abridged. Accepted for publication in A&A.Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts, , , , and . (2019)cite arxiv:1909.12309Comment: 17 pages, 5 figures, 2 appendices.Unveiling the Universe with Emerging Cosmological Probes, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2201.07241Comment: Invited review article for Living Reviews in Relativity. 192 pages, 51 figures, 9 tables.AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN, , , and . (2016)cite arxiv:1606.05648Comment: 21 pages, 10 figures, submitted to the ApJ. The AGNfitter python code is publicly available at https://github.com/GabrielaCR/AGNfitter.