Afterglow radiation in gamma-ray bursts (GRB), extending from the radio band to GeV
energies, is produced as a result of the interaction between the relativistic jet and the …

Over half a century from the discovery of gamma-ray bursts (GRBs), the dominant radiation
mechanism responsible for their bright and highly variable prompt emission remains poorly …

This is the first in a collection of three papers introducing the science with an ultra-violet (UV)
space telescope on an approximately 130 kg small satellite with a moderately fast re …

X-ray flares are generally believed to be produced by the reactivation of the central engine,
and may have the same energy dissipation mechanism as the prompt emission of gamma …

Testing the Universality of Self-organized Criticality in Galactic, Extragalactic, and Black Hole
Systems - IOPscience Skip to content IOP Science home Accessibility Help Search all IOPscience …

Gamma-ray bursts (GRBs) are the most luminous electromagnetic burst in the Universe.
They occur when a rapidly rotating massive star collapses or a binary neutron star merges …

The variability in multi-pulse gamma-ray bursts (GRBs) may help to reveal the mechanism of
underlying processes from the central engine. To investigate whether the self-organized …

We work on a GRB sample whose initial Lorentz factors (Γ 0) are constrained by the
afterglow onset method and the jet opening angles (θ j) are determined by the jet break time …

One of the most surprising gamma-ray burst (GRB) features discovered with the Swift X-ray
telescope (XRT) is a plateau phase in the early X-ray afterglow light curves. These plateaus …

In this paper, we present PyBlastAfterglow, a modular C++ code with a Python interface to
model light curves and sky maps of gamma-ray burst afterglows. The code is open-source …