Discovery of a Protocluster Associated with a Lyα Blob Pair at z = 2.3

Toma Bǎdescu, Yujin Yang, Frank Bertoldi, Ann Zabludoff, Alexander Karim, Benjamin Magnelli

Research output: Contribution to journalArticle

9 Scopus citations

Abstract

Bright Lyα blobs (LABs) - extended nebulae with sizes of ∼100 kpc and Lyα luminosities of ∼1044 erg s-1 - often reside in overdensities of compact Lyα emitters (LAEs) that may be galaxy protoclusters. The number density, variance, and internal kinematics of LABs suggest that they themselves trace group-like halos. Here, we test this hierarchical picture, presenting deep, wide-field Lyα narrowband imaging of a 1° ×0.°5 region around a LAB pair at z = 2.3 discovered previously by a blind survey. We find 183 Lyα emitters, including the original LAB pair and three new LABs with Lyα luminosities of erg s-1 and isophotal areas of 16-24 arcsec2. Using the LAEs as tracers and a new kernel density estimation method, we discover a large-scale overdensity (Boötes J1430+3522) with a surface density contrast of δ, a volume density contrast of δ ∼10.4, and a projected diameter of ≈20 comoving Mpc. Comparing with cosmological simulations, we conclude that this LAE overdensity will evolve into a present-day Coma-like cluster with log(M/M) ∼ 15.1 ± 0.2. In this and three other wide-field LAE surveys re-analyzed here, the extents and peak amplitudes of the largest LAE overdensities are similar, not increasing with survey size, and implying that they were indeed the largest structures then and today evolve into rich clusters. Intriguingly, LABs favor the outskirts of the densest LAE concentrations, i.e., intermediate LAE overdensities of . We speculate that these LABs mark infalling protogroups being accreted by the more massive protocluster.

Original languageEnglish (US)
Article number172
JournalAstrophysical Journal
Volume845
Issue number2
DOIs
StatePublished - Aug 20 2017

Keywords

  • galaxies: clusters: general
  • galaxies: formation
  • galaxies: high-redshift
  • intergalactic medium
  • large-scale structure of universe

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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