Saraswati: An Extremely Massive ~ 200 Megaparsec Scale Supercluster

TL;DR

The paper reports the discovery of Saraswati, an extremely massive supercluster spanning over 200 Mpc at redshift 0.3, providing insights into large-scale structure formation and the role of dark energy.

Contribution

It presents the identification and detailed characterization of Saraswati, one of the largest known superclusters, and discusses its implications for cosmology and structure formation models.

Findings

Saraswati spans at least 200 Mpc and contains at least 43 galaxy clusters.

The supercluster's mass is approximately 2 x 10^16 solar masses.

Its properties challenge and inform models of large-scale structure formation.

Abstract

Here we report the discovery of an extremely massive and large supercluster (called Saraswati) found in the Stripe 82 region of SDSS. This supercluster is a major concentration of galaxies and galaxy clusters, forming a wall-like structure spanning at least 200 Mpc across at the redshift $z \approx 0.3$. This enormous structure is surrounded by a network of galaxy filaments, clusters, and large, $\sim40 - 170$ Mpc diameter, voids. The mean density contrast $\delta$ (relative to the background matter density of the universe) of Saraswati is $\gtrsim 1.62$ and the main body of the supercluster comprises at least 43 massive galaxy clusters (mean $z = 0.28$) with a total mass of $\sim 2 \times 10^{16} M_{\odot}$. The spherical collapse model suggests that the central region of radius $\sim20$ Mpc and mass at least $ 4 \times 10^{15} M_{\odot}$ may be collapsing. This places it among the few largest and most massive superclusters known, comparable to the most massive `Shapley Concentration' ($z \approx 0.046$) in the nearby universe. The Saraswati supercluster and its environs reveal that some extreme large-scale, prominent matter density enhancements had formed $\sim4$ Gy in the past when dark energy had just started to dominate structure formation. This galactic concentration sheds light on the role of dark energy and cosmological initial conditions in supercluster formation, and tests the competing cosmological models.