Kavli Affiliate: Claudio Ricci | First 5 Authors: , , , , | Summary: 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. The SDSS-V is providing optical spectroscopy for samples of […]
Continue.. X-ray selected broad absorption line quasars in SDSS-V: BALs and non-BALs span the same range of X-ray properties