Hiremath, Pranavi; Rankine, Amy L; Aird, James; Brandt, W. N; Hidalgo, Paola Rodriguez; Anderson, S. F; Aydar, Catarina; Ricci, Claudio; Schneider, D. P; Vivek, M; Igo, Zsofi; Morrison, Sean; Salvato, Mara
(Oxford University Press on behalf of Royal Astronomical Society, 2025-09)
Broad absorption line (BAL) quasars are often considered X-ray weak relative to their optical/UV luminosity, whether intrinsically (i.e. the coronal emission is fainter) or due to large column densities of absorbing material. ...