The X-ray properties of <i>z</i> &gt; 6 quasars: no evident evolution of accretion physics in the first Gyr of the Universe

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dc.contributor.authorVito, F.
dc.contributor.authorBrandt, W. N.
dc.contributor.authorBauer, F. E.
dc.contributor.authorCalura, F.
dc.contributor.authorGilli, R.
dc.contributor.authorLuo, B.
dc.contributor.authorShemmer, O.
dc.contributor.authorVignali, C.
dc.contributor.authorZamorani, G.
dc.contributor.authorBrusa, M.
dc.contributor.authorCivano, F.
dc.contributor.authorComastri, A.
dc.contributor.authorNanni, R.
dc.date.accessioned2025-01-23T19:58:04Z
dc.date.available2025-01-23T19:58:04Z
dc.date.issued2019
dc.description.abstractContext. X-ray emission from quasars (QSOs) has been used to assess supermassive black hole accretion properties up to z approximate to 6. However, at z > 6 only approximate to 15 QSOs are covered by sensitive X-ray observations, preventing a statistically significant investigation of the X-ray properties of the QSO population in the first Gyr of the Universe.
dc.description.abstractAims. We present new Chandra observations of a sample of 10 z > 6 QSOs, selected to have virial black-hole mass estimates from Mg II line spectroscopy (logM(BH)/M-circle dot = 8.5-9.6). Adding archival X-ray data for an additional 15 z > 6 QSOs, we investigate the X-ray properties of the QSO population in the first Gyr of the Universe. In particular, we focus on the L-UV-L-X relation, which is traced by the alpha(ox) parameter, and the shape of their X-ray spectra.
dc.description.abstractMethods. We performed photometric analyses to derive estimates of the X-ray luminosities of our z > 6 QSOs, and thus their alpha(ox) values and bolometric corrections (K-bol = L-bol/L-X). We compared the resulting alpha(ox) and K-bol distributions with the results found for QSO samples at lower redshift, and ran several statistical tests to check for a possible evolution of the L-UV-L-X relation. Finally, we performed a basic X-ray spectral analysis of the brightest z > 6 QSOs to derive their individual photon indices, and joint spectral analysis of the whole sample to estimate the average photon index.
dc.description.abstractResults. We detect seven of the new Chandra targets in at least one standard energy band, while two more are detected discarding energies E > 5 keV, where background dominates. We confirm a lack of significant evolution of alpha(ox) with redshift, which extends the results from previous works up to z > 6 with a statistically significant QSO sample. Furthermore, we confirm the trend of an increasing bolometric correction with increasing luminosity found for QSOs at lower redshifts. The average power-law photon index of our sample (<Gamma > = 2.20(-0.34)(+0.39) and <Gamma > = 2.13(-0.13)(+0.13) for sources with < 30 and >30 net counts, respectively) is slightly steeper than, but still consistent with, typical QSOs at z = 1 - 6.
dc.description.abstractConclusions. All of these results indicate a lack of substantial evolution of the inner accretion-disk and hot-corona structure in QSOs from low redshift to z > 6. Our data hint at generally high Eddington ratios at z > 6.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/201936217
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201936217
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/100753
dc.identifier.wosidWOS:000516616500001
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectmethods: data analysis
dc.subjectgalaxies: active
dc.subjectgalaxies: nuclei
dc.subjectX-rays: galaxies
dc.subjectgalaxies: high-redshift
dc.subjectquasars: general
dc.titleThe X-ray properties of <i>z</i> &gt; 6 quasars: no evident evolution of accretion physics in the first Gyr of the Universe
dc.typeartículo
dc.volumen630
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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