Active galactic nuclei are primarily powered by a supermassive black hole lying at the center of a host galaxy that is accreting matter from its vicinity. The radiation from the central source ionizes the inner dense gas, the so-called broad-line region. Using the Gemini Near-Infrared Spectrograph on the Gemini North telescope, one half of the International Gemini Observatory, operated by NSF’s NOIRLab, astronomers have detected two near-infrared...
