Galaxy protocluster candidates around z ~ 2.4 radio galaxies

TL;DR

This study investigates the environments of six high-redshift radio galaxies, revealing significant galaxy overdensities that are likely protoclusters, with most galaxies actively forming stars and potential to evolve into galaxy clusters.

Contribution

First detailed analysis of galaxy overdensities around z ~ 2.4 radio galaxies, identifying candidate protoclusters with properties consistent with future galaxy clusters.

Findings

Three radio galaxies are surrounded by significant galaxy overdensities.

Overdensities have masses exceeding 10^14 solar masses, likely collapsing into virialized structures.

Protocluster galaxies predominantly exhibit blue, star-forming characteristics.

Abstract

We study the environments of 6 radio galaxies at 2.2 < z < 2.6 using wide-field near-infrared images. We use colour cuts to identify galaxies in this redshift range, and find that three of the radio galaxies are surrounded by significant surface overdensities of such galaxies. The excess galaxies that comprise these overdensities are strongly clustered, suggesting they are physically associated. The colour distribution of the galaxies responsible for the overdensity are consistent with those of galaxies that lie within a narrow redshift range at z ~ 2.4. Thus the excess galaxies are consistent with being companions of the radio galaxies. The overdensities have estimated masses in excess of 10^14 solar masses, and are dense enough to collapse into virizalised structures by the present day: these structures may evolve into groups or clusters of galaxies. A flux-limited sample of protocluster galaxies with K < 20.6 mag is derived by statistically subtracting the fore- and background galaxies. The colour distribution of the protocluster galaxies is bimodal, consisting of a dominant blue sequence, comprising 77 +/- 10% of the galaxies, and a poorly populated red sequence. The blue protocluster galaxies have similar colours to local star-forming irregular galaxies (U -V ~ 0.6), suggesting most protocluster galaxies are still forming stars at the observed epoch. The blue colours and lack of a dominant protocluster red sequence implies that these cluster galaxies form the bulk of their stars at z < 3.