Kavli Affiliate: Roberto Maiolino | Summary:We test whether "little red dots” (LRDs) are the dust-reddened, high-inclination counterparts of bluer compact broad-line active galactic nuclei, here referred to as "little blue dots” (LBDs), by modeling their relative number densities and luminosities. Using the observed UV luminosity function (LF) of broad-line active galactic nuclei (BLAGNs) at z>4 […]
Continue.. Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses