A Giant Arc on the Sky
Alexia M. Lopez, Roger G. Clowes, Gerard M. Williger

TL;DR
This paper reports the discovery of an enormous, nearly symmetrical large-scale structure at redshift 0.8, identified through MgII absorbers, challenging assumptions of the Cosmological Principle and expanding understanding of cosmic structures.
Contribution
It introduces a novel approach using MgII absorbers to detect large-scale structures at intermediate redshifts, revealing one of the largest known cosmic structures.
Findings
The Giant Arc spans approximately 1 Gpc in size.
Statistical analyses confirm the structure's significance at over 3 sigma.
The structure's overdensity is about 1.3 ± 0.3.
Abstract
We present the serendipitous discovery of a `Giant Arc on the Sky' at . The Giant Arc (GA) spans Gpc (proper size, present epoch), and appears to be almost symmetrical on the sky. It was discovered via intervening MgII absorbers in the spectra of background quasars, using the catalogues of Zhu \& M\'enard. The use of MgII absorbers represents a new approach to the investigation of large-scale structures (LSSs) at redshifts . We present the observational properties of the GA, and we assess it statistically using methods based on: (i) single-linkage hierarchical clustering (); (ii) the Cuzick-Edwards test (); and (iii) power spectrum analysis (). Each of these methods has distinctive attributes and powers, and we advise considering the evidence from the ensemble. We discuss our approaches…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Electrical and Electromagnetic Research
