Detection of a huge explosion in the early Universe
G. Cusumano, V. Mangano, G. Chincarini, A. Panaitescu, D.N. Burrows,, V. La Parola, T. Sakamoto, S. Campana, T. Mineo, G. Tagliaferri, L. Angelini,, S.D. Barthelemy, A.P. Beardmore, P.T. Boyd, L. Cominsky, C. Gronwall, E.E., Fenimore, N. Gehrels, P. Giommi, M. Goad, K. Hurley

TL;DR
This paper reports the discovery of the most distant gamma-ray burst at redshift 6.29, providing insights into early universe star formation and the re-ionization era, and demonstrating the potential of GRBs as probes of the early cosmos.
Contribution
It presents the first observation of a gamma-ray burst at such a high redshift, revealing the existence of massive stars shortly after the Big Bang.
Findings
The gamma-ray burst occurred 700 million years after the Big Bang.
It confirms the presence of massive stars in the early universe.
The burst's redshift of 6.29 makes it the most distant observed so far.
Abstract
Gamma-ray Bursts (GRBs) are bright flashes of high energy photons that can last from about 10 milliseconds to 10 minutes. Their origin and nature have puzzled the scientific community for about 25 years until 1997, when the first X-ray afterglows of long (> 2 s duration) bursts were detected and the first optical and radio counterparts were found. These measurements established that long GRBs are typically at high redshift (z 1.6) and are in sub-luminous star-forming host galaxies. They are likely produced in core-collapse explosions of a class of massive stars that give rise to highly relativistic jets (collapsar model). Internal inhomogeneities in the velocity field of the relativistic expanding flow lead to collisions between fast moving and slow moving fluid shells and to the formation of internal shock waves. These shocks are believed to produce the observed prompt emission in the…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysical Phenomena and Observations
