Alignments of Galaxy Group Shapes with Large Scale Structure

TL;DR

This study investigates how galaxy groups align with the large-scale structure of the universe, revealing a strong mass-dependent alignment consistent with cosmological simulations and gravitational instability theories.

Contribution

It extends the two-point cross-correlation function to quantify galaxy group alignments with large-scale structures, providing observational evidence supporting cosmological models.

Findings

Strong alignment signal up to 30 Mpc/h

Alignment increases with galaxy group mass

Results agree with LCDM cosmological simulations

Abstract

In this paper we analyse the alignment of galaxy groups with the surrounding large scale structure traced by spectroscopic galaxies from the Sloan Digital Sky Survey Data Release 7. We characterise these alignments by means of an extension of the classical two-point cross-correlation function, developed by Paz et al. 2008 (arXiv:0804.4477, MNRAS 389 1127). We find a strong alignment signal between the projected major axis of group shapes and the surrounding galaxy distribution up to scales of 30 Mpc/h. This observed anisotropy signal becomes larger as the galaxy group mass increases, in excellent agreement with the corresponding predicted alignment obtained from mock catalogues and LCDM cosmological simulations. These measurements provide new direct evidence of the adequacy of the gravitational instability picture to describe the large-scale structure formation of our Universe.