SDSS-V: Revealing a weak accretion state in X-ray selected red quasars

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ID: 322997
2026
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Abstract
Abstract Red quasars (rQSOs) have been recognized as a short-lived stage in the evolutionary cycle of Active Galactic Nuclei (AGN), with fundamental differences in their intrinsic properties compared to blue quasars (bQSOs). We present the first large X-ray sample of 380 rQSOs, selected from the eROSITA/SDSS-V collaboration, providing uniform X-ray detection with optical spectroscopy across half the sky. We combine X-ray imaging, optical spectroscopy, and multi-wavelength photometry to probe the accretion, absorption, spectroscopic, and host properties of rQSOs compared to a bQSO sample. Independent Component Analysis is used to reconstruct optical spectra in a data-driven approach while accounting for dust reddening and host contamination. rQSOs are intrinsically X-ray fainter than bQSOs, with a higher fraction found at lower X-ray luminosities. We investigate the relative X-ray strength of rQSOs by measuring the spectral slope indicator αOX. Despite their suppressed X-ray emission, rQSOs are not optically faint, but show low αOX values and higher dust-corrected optical luminosities, indicating weak X-ray emission relative to their bright optical continua. X-ray spectral measurements reveal large gas column densities relative to optical reddening due to dust, implying that X-ray absorption could arise from dust-free gas close to the supermassive Black Hole (BH) rather than a classical dusty torus, while the dust responsible for optical reddening likely resides on host-galaxy scales or is associated with dusty gas carried in disc winds. rQSOs trace a phase of suppressed BH assembly relative to stellar mass growth, suggesting that they may represent a distinct evolutionary stage where BH accretion is suppressed while the host galaxy continues to grow.
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openalex_W7171832796 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Paloma Guetzoyan, James Aird, Amy L. Rankine, Stephanie LaMassa, Peter Breiding, M. Salvato, Johannes Buchner, Z. Igo, Roberto J Assef, Hector Ibarra-Medel, Catarina Aydar, C. A. Negrete, Claudio Ricci, W N Brandt, Dong‐Woo Kim, Dominika Wylezalek, Scott F Anderson, Donald P Schneider, Delvin Demke, Anton M. Koekemoer
Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1438
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