机译:红移4.6的高光遮盖类星体的多重合并程序集
Univ Diego Portales, Fac Ingn & Ciencias, Nucleo Astron, Ejercito Libertador 441, Santiago 8320000, Chile;
Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England;
Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA;
Univ Lyon 1, Ctr Rech Astrophys Lyon, Ecole Normale Super Lyon, Univ Lyon,UMR5574,CNRS, F-69230 St Genis Laval, France;
Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England;
Korea Inst Adv Study, Sch Phys, 85 Hoegiro, Seoul 02455, South Korea;
Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China;
MIT, Dept Phys, 77 Massachusetts Ave, Cambridge, MA 02139 USA;
CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA;
机译:REDSHIFTS〜0.5–3时,严重遮挡,超亮类星体的无线电射流反馈和恒星形成。 I.阿尔玛观测
机译:WISE选出的高发光,尘埃模糊的星系在z〜2.3时的隐藏类星体核
机译:最明亮的重模遮掩的类星体具有高合并分数:明智的热尘遮挡星系的形态学研究
机译:红移Z〜2的遮挡Quasars
机译:红移2
机译:类星体的X射线光度-红移关系
机译:在Redshift 4.6的超闪光灯模糊的Quasar的多项合并组合