A Large Scale Structure at Redshift 1.71 in the Lockman Hole
Abstract
We previously identified LH146, a diffuse X-ray source in the Lockman Hole, as a galaxy cluster at redshift 1.753. The redshift was based on one spectroscopic value, buttressed by seven additional photometric redshifts. We here confirm the previous spectroscopic redshift and present concordant spectroscopic redshifts for an additional eight galaxies. The average of these nine redshifts is 1.714 +/- 0.012 (error on mean). Scrutiny of the galaxy distribution in redshift and the plane of the sky shows that there are two concentrations of galaxies near the X-ray source. In addition there are three diffuse X-ray sources spread along the axis connecting the galaxy concentrations. LH146 is one of these three and lies approximately at the center of the two galaxy concentrations and the outer two diffuse X-ray sources. We thus conclude that LH146 is at the redshift initially reported but it is not a single virialized galaxy cluster as previously assumed. Rather it appears to mark the approximate center of a larger region containing more objects. For brevity we term all these objects and their alignments as large scale structure. The exact nature of LH146 itself remains unclear.
Keywords
Cite
@article{arxiv.1311.2201,
title = {A Large Scale Structure at Redshift 1.71 in the Lockman Hole},
author = {J. P. Henry and K. Aoki and A. Finoguenov and S. Fotopoulou and G. Hasinger and M. Salvato and H. Suh and M. Tanaka},
journal= {arXiv preprint arXiv:1311.2201},
year = {2015}
}
Comments
22 pages, 15 figures, accepted for publication in the Astrophysical Journal