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- W3124803336 abstract "We report on deep XMM-Newton and NuSTAR observations of the high redshift, z=2.94, extremely red quasar (ERQ), SDSS J165202.60+172852.4, with known galactic ionized outflows detected via spatially-resolved [OIII] emission lines. X-ray observations allow us to directly probe the accretion disk luminosity and the geometry and scale of the circumnuclear obscuration. We fit the spectra from the XMM-Newton/EPIC and NuSTAR detectors with a physically motivated torus model and constrain the source to exhibit a near Compton-thick column density of $N_H=(1.02^{+0.76}_{-0.41})times10^{24}textrm{ cm}^{-2}$, a near edge-on geometry with the line-of-sight inclination angle of $theta_i=85^{circ}$, and a scattering fraction of $f_{sc}sim 3$ %. The absorption-corrected, intrinsic 2-10 keV X-ray luminosity of $L_{textrm{2-10}}=(1.4^{+1}_{-1}) times10^{45} textrm{ erg s}^{-1}$ reveals a powerful quasar that is not intrinsically X-ray weak, consistent with observed trends in other ERQs. We also estimate the physical properties of the obscuration, although highly uncertain: the warm ionized scattering density of $n_e sim 7.5times(10^2-10^3)textrm{ cm}^{-3}$ and the obscuration mass of $M_{obsc} sim 1.7times(10^4-10^6) M_{odot}$. As previously suggested with shallower X-ray observations, optical and infrared selection of ERQ has proved effective in finding obscured quasars with powerful outflow signatures. Our observations provide an in-depth view into the X-ray properties of ERQs and support the conclusions of severely photon-limited studies of obscured quasar populations at high redshifts." @default.
- W3124803336 created "2021-02-01" @default.
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- W3124803336 date "2021-01-20" @default.
- W3124803336 modified "2023-10-18" @default.
- W3124803336 title "X-ray analysis of SDSS J165202.60+172852.4, an obscured quasar with outflows at peak galaxy formation epoch" @default.
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- W3124803336 doi "https://doi.org/10.1093/mnras/stab137" @default.
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