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Discovery and characterization of 25 new quasars at 4.6 < z < 6.9 from wide-field multiband surveys
Luminous quasars at z>4 provide key insights into the early Universe. Their rarity necessitates wide-field multiband surveys to efficiently separate them from the main astrophysical contaminants (i.e., ultracool dwarfs). To expand the sample of high-z quasars, we conducted targeted selections usi
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