Two close large quasar groups of size ∼ 350 Mpc at 
Article first published online: 3 NOV 2011
DOI: 10.1111/j.1365-2966.2011.19719.x
© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS
Issue

Monthly Notices of the Royal Astronomical Society
Volume 419, Issue 1, pages 556–565, January 2012
Additional Information
How to Cite
Clowes, R. G., Campusano, L. E., Graham, M. J. and Söchting, I. K. (2012), Two close large quasar groups of size ∼ 350 Mpc at
. Monthly Notices of the Royal Astronomical Society, 419: 556–565. doi: 10.1111/j.1365-2966.2011.19719.x
Publication History
- Issue published online: 13 DEC 2011
- Article first published online: 3 NOV 2011
- Accepted 2011 August 27. Received 2011 August 26; in original form 2011 August 2
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Keywords:
- galaxies: clusters: general;
- quasars: general;
- large-scale structure of Universe
ABSTRACT
The Clowes & Campusano large quasar group (LQG) at
has been re-examined using the quasar data from the DR7QSO catalogue of the Sloan Digital Sky Survey. In the 1991 discovery, the LQG impinged on the northern, southern and eastern limits of the survey. In the DR7QSO data, the western, northern and southern boundaries of the LQG remain essentially the same, but an extension eastwards of ∼2° is indicated. In the DR7QSO data, the LQG has 34 members, with
. A new group of 38 members is indicated at
and within ∼2
0 of the Clowes & Campusano LQG. The characteristic sizes of these two LQGs, ∼350–400 Mpc, appear to be only marginally consistent with the scale of homogeneity in the concordance cosmology. In addition to their intrinsic interest, these two LQGs provide locations in which to investigate early large-scale structure in galaxies and to identify high-z clusters. A method is presented for assessing the statistical significance and overdensity of groups found by linkage of points.

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