Properties of Gamma Ray Bursts at different redshifts
G. Pizzichini, E. Maiorano, M. Genghini, F. Munz
TL;DR
This paper investigates how the properties of gamma-ray bursts vary with redshift, aiming to understand potential differences related to their distance or observational factors.
Contribution
It analyzes restframe properties of GRBs across different redshifts to identify possible variations linked to distance or observational effects.
Findings
Identified potential differences in GRB properties at various redshifts
Explored correlations between redshift and observed GRB characteristics
Provided insights into how observational conditions affect GRB measurements
Abstract
GRBs are now detected up to z = 8.26 . We try to find differences, in their restframe properties, which could be related either to distance or to observing conditions.
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Taxonomy
TopicsGamma-ray bursts and supernovae