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Discovery of a Clustered Quasar Pair at z ≈ 5: Biased Peaks in Early Structure Formation*

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S. G. Djorgovski1, D. Stern2, A. A. Mahabal1 and R. Brunner1,3

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[1]

Gas distribution, metal enrichment and baryon fraction in Gaussian and non-Gaussian universes

Umberto Maio  Classical and Quantum Gravity 2011  28 225015
IOPscience 
[2]

A Large Number of z > 6 Galaxies Around a QSO at z = 6.43: Evidence for a Protocluster?

Yousuke Utsumi et al.  The Astrophysical Journal 2010  721 1680
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[3]

Binary Quasars at High Redshift. I. 24 New Quasar Pairs at z ~ 3-4

Joseph F. Hennawi et al.  The Astrophysical Journal 2010  719 1672
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[4]

The Environments of High-Redshift Quasi-Stellar Objects

Soyoung Kim et al.  The Astrophysical Journal 2009  695 809
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[5]

Clustering of High-Redshift (z ≥ 2.9) Quasars from the Sloan Digital Sky Survey

Yue Shen et al.  The Astronomical Journal 2007  133 2222
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[6]

Searching High-Redshift Large-Scale Structures: Photometry of Four Fields around Quasar Pairs at z ~ 1

N. V. Boris et al.  The Astrophysical Journal 2007  666 747
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[7]

The Discovery of Three New z > 5 Quasars in the AGN and Galaxy Evolution Survey

Richard J. Cool et al.  The Astronomical Journal 2006  132 823
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[8]

Binary Quasars in the Sloan Digital Sky Survey: Evidence for Excess Clustering on Small Scales

Joseph F. Hennawi et al.  The Astronomical Journal 2006  131 1
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[9]

Clustering of Star-forming Galaxies Near a Radio Galaxy at z = 5.2

Roderik A. Overzier et al.  The Astrophysical Journal 2006  637 58
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[10]

Discovery of an Optically Faint Quasar at z = 5.70 and Implications for the Faint Endof the Quasar Luminosity Function

A. Mahabal et al  The Astrophysical Journal Letters 2005  634 L9
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[11]

Evidence of Primordial Clustering around the QSO SDSS J1030+0524 at z = 6.28

M. Stiavelli et al  The Astrophysical Journal Letters 2005  622 L1
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[12]

The X-Ray Spectral Properties and Variability of Luminous High-Redshift Active Galactic Nuclei

O. Shemmer et al.  The Astrophysical Journal 2005  630 729
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  2. Stellar Masses of Lyman Break Galaxies, Lyα Emitters, and Radio Galaxies in Overdense Regions at z = 4-6

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