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• W3136900550 endingPage "A133" @default.
• W3136900550 startingPage "A133" @default.
• W3136900550 abstract "Context. The discovery of hundreds of quasi-stellar objects (QSOs) in the first gigayear of the Universe powered by already grown supermassive black holes (SMBHs) challenges our knowledge of SMBH formation. In particular, investigations of z > 6 QSOs that present notable properties can provide unique information on the physics of fast SMBH growth in the early Universe. Aims. We present the results of follow-up observations of the z = 6.515 radio-quiet QSO PSO167–13, which is interacting with a close companion galaxy. The PSO167–13 system has recently been proposed to host the first heavily obscured X-ray source at high redshift. The goals of these new observations are to confirm the existence of the X-ray source and to investigate the rest-frame UV properties of the QSO. Methods. We observed the PSO167–13 system with Chandra /ACIS-S (177 ks) and obtained new spectroscopic observations (7.2 h) with Magellan /FIRE. Results. No significant X-ray emission is detected from the PSO167–13 system, suggesting that the obscured X-ray source previously tentatively detected was either due to a strong background fluctuation or is highly variable. The upper limit (90% confidence level) on the X-ray emission of PSO167–13 ( L 2−10 keV < 8.3 × 10 43 erg s −1 ) is the lowest available for a z > 6 QSO. The ratio between the X-ray and UV luminosity of α ox < −1.95 makes PSO167–13 a strong outlier from the α ox − L UV and L X − L bol relations. In particular, its X-ray emission is more than six times weaker than the expectation based on its UV luminosity. The new Magellan /FIRE spectrum of PSO167–13 is strongly affected by unfavorable sky conditions, but the tentatively detected C IV and Mg II emission lines appear strongly blueshifted. Conclusions. The most plausible explanations for the X-ray weakness of PSO167–13 are intrinsic weakness or small-scale absorption by Compton-thick material. The possible strong blueshift of its emission lines hints at the presence of nuclear winds, which could be related to its X-ray weakness." @default.
• W3136900550 created "2021-03-29" @default.
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• W3136900550 date "2021-05-01" @default.
• W3136900550 modified "2023-10-18" @default.
• W3136900550 title "<i>Chandra</i> and <i>Magellan</i>/FIRE follow-up observations of PSO167–13: An X-ray weak QSO at <i>z</i> = 6.515" @default.
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