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Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses
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 (
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