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Quasar UV Luminosity Function at $3.5 postprint

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Abstract: We present a well-designed sample of more than 1000 type 1 quasars at $3.50.5$. The evolution of the QLFs from $z\sim5$ to $3.5$ can be described by a pure density evolution model ($\propto10^{kz}$) and the parameter $k$ is similar to that at $5

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[V1] 2023-02-19 20:58:59 ChinaXiv:202303.06547V1 Download

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