  Context. Research over the past three decades has revolutionized cosmology
while supporting the standard cosmological model. However, the cosmological
principle of Universal homogeneity and isotropy has always been in question,
since structures as large as the survey size have always been found each time
the survey size has increased. Until 2013, the largest known structure in our
Universe was the Sloan Great Wall, which is more than 400 Mpc long located
approximately one billion light years away.
  Aims. Gamma-ray bursts are the most energetic explosions in the Universe. As
they are associated with the stellar endpoints of massive stars and are found
in and near distant galaxies, they are viable indicators of the dense part of
the Universe containing normal matter. The spatial distribution of gamma-ray
bursts can thus help expose the large scale structure of the Universe.
  Methods. As of July 2012, 283 GRB redshifts have been measured. Subdividing
this sample into nine radial parts, each containing 31 GRBs, indicates that the
GRB sample having 1.6 < z < 2.1 differs significantly from the others in that
14 of the 31 GRBs are concentrated in roughly 1/8 of the sky. A two-dimensional
Kolmogorov-Smirnov test, a nearest-neighbour test, and a Bootstrap Point-Radius
Method explore the significance of this clustering.
  Results. All tests used indicate that there is a statistically significant
clustering of the GRB sample at 1.6 < z < 2.1. Furthermore, this angular excess
cannot be entirely attributed to known selection biases, making its existence
due to chance unlikely.
  Conclusions. This huge structure lies ten times farther away than the Sloan
Great Wall, at a distance of approximately ten billion light years. The size of
the structure defined by these GRBs is about 2000-3000 Mpc, or more than six
times the size of the Sloan Great Wall.
