Cosmological simulations suggest a strong correlation between high
optical-depth Ly$\alpha$ absorbers, which arise from the intergalactic medium
(IGM), and 3-D mass overdensities on scales of $10-30$ $h^-1$ comoving Mpc.
By examining the absorption spectra of $\sim$ 80,000 QSO sight-lines over a
volume of 0.1 Gpc$^3$ in the Sloan Digital Sky Survey III (SDSS-III), we have
identified an extreme overdensity, BOSS1441, which contains a rare group of
strong Ly$\alpha$ absorbers at $z=2.320.02$. 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 Ly$\alpha$ emitters
(LAEs) down to $0.7L_Ly\alpha^*$, and reveal a large-scale
structure of Ly$\alpha$ 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
$10.82.6$ on a 15 comoving Mpc scale which could collapse to a massive
cluster with $M\gtrsim10^15$ M$_ødot$ at $z\sim0$. This overdensity is among
the most massive large-scale structures at $z\sim2$ discovered to date.
Description
[1609.02913] MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at $z=2.32$
%0 Generic
%1 cai2016mapping
%A Cai, Zheng
%A Fan, Xiaohui
%A Bian, Fuyan
%A Zabludoff, Ann
%A Yang, Yujin
%A Prochaska, J. Xavier
%A McGreer, Ian
%A Zheng, Zhen-Ya
%A Kashikawa, Nobunari
%A Wang, Ran
%A Frye, Brenda
%A Green, Richard
%A Jiang, Linhua
%D 2016
%K cluster igm lya overdensity qsos
%T MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an
Extremely Massive Overdensity BOSS1441 at $z=2.32$
%U http://arxiv.org/abs/1609.02913
%X Cosmological simulations suggest a strong correlation between high
optical-depth Ly$\alpha$ absorbers, which arise from the intergalactic medium
(IGM), and 3-D mass overdensities on scales of $10-30$ $h^-1$ comoving Mpc.
By examining the absorption spectra of $\sim$ 80,000 QSO sight-lines over a
volume of 0.1 Gpc$^3$ in the Sloan Digital Sky Survey III (SDSS-III), we have
identified an extreme overdensity, BOSS1441, which contains a rare group of
strong Ly$\alpha$ absorbers at $z=2.320.02$. 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 Ly$\alpha$ emitters
(LAEs) down to $0.7L_Ly\alpha^*$, and reveal a large-scale
structure of Ly$\alpha$ 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
$10.82.6$ on a 15 comoving Mpc scale which could collapse to a massive
cluster with $M\gtrsim10^15$ M$_ødot$ at $z\sim0$. This overdensity is among
the most massive large-scale structures at $z\sim2$ discovered to date.
@misc{cai2016mapping,
abstract = {Cosmological simulations suggest a strong correlation between high
optical-depth Ly$\alpha$ absorbers, which arise from the intergalactic medium
(IGM), and 3-D mass overdensities on scales of $10-30$ $h^{-1}$ comoving Mpc.
By examining the absorption spectra of $\sim$ 80,000 QSO sight-lines over a
volume of 0.1 Gpc$^3$ in the Sloan Digital Sky Survey III (SDSS-III), we have
identified an extreme overdensity, BOSS1441, which contains a rare group of
strong Ly$\alpha$ absorbers at $z=2.32\pm 0.02$. 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 Ly$\alpha$ emitters
(LAEs) down to $0.7\times L_{\rm{Ly\alpha}}^*$, and reveal a large-scale
structure of Ly$\alpha$ 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
$10.8\pm 2.6$ on a 15 comoving Mpc scale which could collapse to a massive
cluster with $M\gtrsim10^{15}$ M$_\odot$ at $z\sim0$. This overdensity is among
the most massive large-scale structures at $z\sim2$ discovered to date.},
added-at = {2016-09-13T10:36:15.000+0200},
author = {Cai, Zheng and Fan, Xiaohui and Bian, Fuyan and Zabludoff, Ann and Yang, Yujin and Prochaska, J. Xavier and McGreer, Ian and Zheng, Zhen-Ya and Kashikawa, Nobunari and Wang, Ran and Frye, Brenda and Green, Richard and Jiang, Linhua},
biburl = {https://www.bibsonomy.org/bibtex/2dc6428a709a734da36ec6f6e04fd6507/miki},
description = {[1609.02913] MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at $z=2.32$},
interhash = {c0c41cf76465ed56773880ddd64bddd9},
intrahash = {dc6428a709a734da36ec6f6e04fd6507},
keywords = {cluster igm lya overdensity qsos},
note = {cite arxiv:1609.02913Comment: 12 pages, 8 figures. submitted to ApJ, Comments are welcome},
timestamp = {2016-09-13T10:36:15.000+0200},
title = {MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an
Extremely Massive Overdensity BOSS1441 at $z=2.32$},
url = {http://arxiv.org/abs/1609.02913},
year = 2016
}