您当前的位置: > 详细浏览

Quasar UV Luminosity Function at $3.5 后印本

请选择邀稿期刊:
摘要: 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

版本历史

[V1] 2023-02-19 20:58:59 ChinaXiv:202303.06547V1 下载全文

点击下载全文
预览
同行评议状态
待评议
许可声明
metrics指标
  •  点击量932
  •  下载量80
评论
分享