309 research outputs found

    MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at z=2.32z=2.32

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    Cosmological simulations suggest a strong correlation between high optical-depth Lyα\alpha absorbers, which arise from the intergalactic medium (IGM), and 3-D mass overdensities on scales of 103010-30 h1h^{-1} comoving Mpc. By examining the absorption spectra of \sim 80,000 QSO sight-lines over a volume of 0.1 Gpc3^3 in the Sloan Digital Sky Survey III (SDSS-III), we have identified an extreme overdensity, BOSS1441, which contains a rare group of strong Lyα\alpha absorbers at z=2.32±0.02z=2.32\pm 0.02. This absorber group is associated with six QSOs at the same redshift on a 30 comoving Mpc scale. Using Mayall/MOSAIC narrowband and broadband imaging, we detect Lyα\alpha emitters (LAEs) down to 0.7×LLyα0.7\times L_{\rm{Ly\alpha}}^*, and reveal a large-scale structure of Lyα\alpha emitters (LAEs) in this field. Our follow-up Large Binocular Telescope (LBT) observations have spectroscopically confirmed 19 galaxies in the density peak. We show that BOSS1441 has an LAE overdensity of 10.8±2.610.8\pm 2.6 on a 15 comoving Mpc scale which could collapse to a massive cluster with M1015M\gtrsim10^{15} M_\odot at z0z\sim0. This overdensity is among the most massive large-scale structures at z2z\sim2 discovered to date.Comment: 12 pages, 8 figures. submitted to ApJ, Comments are welcom
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