Detection of 20–30 h$\mathsf{^{-1}}$ Mpc-scale galaxy structures embedded in 100 h$\mathsf{^{-1}}$ Mpc-scale structures of quasars and MgII absorbers at $\textit{z}\simeq\mathsf{0.8}$ and $\textit{z} \simeq\mathsf{1.2}$

Author:

Haines C. P.,Campusano L. E.,Clowes R. G.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 11 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Compatibility of the Large Quasar Groups with the Concordance Cosmological Model;Monthly Notices of the Royal Astronomical Society;2016-06-26

2. A giant ring-like structure at 0.78 < z < 0.86 displayed by GRBs;Monthly Notices of the Royal Astronomical Society;2015-07-24

3. Two close large quasar groups of size ∼ 350 Mpc at;Monthly Notices of the Royal Astronomical Society;2011-11-03

4. The nature of proximate damped Lyman α systems★;Monthly Notices of the Royal Astronomical Society;2010-05

5. THE CLOWES-CAMPUSANO LARGE QUASAR GROUP SURVEY. I.GALEXSELECTED SAMPLE OF LYMAN BREAK GALAXIES ATz∼ 1;The Astrophysical Journal;2009-08-13

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