XRF 241001A is a low-luminosity collapsar event with a broad-line Type Ic supernova, supporting XRFs as the faint end of the long GRB population observed on-axis by a weak jet.
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GRMHD simulations of GRB 090510 predict energetics and jet opening angles consistent with observations within 1 sigma when jet angles evolve with redshift, while dynamical ejecta influence collimation and a suite of models explores broader GRB properties.
EP250416a is an X-ray-rich long GRB at z=0.963 showing a late jet break at 1.5e6 s and optical darkness explained by A_V^host = 5.5 mag extinction.
citing papers explorer
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XRF 241001A/SN 2024aiiq: A Faint Soft X-ray Transient Detected by SVOM with a Broad-Line Type Ic Supernova Revealed by JWST
XRF 241001A is a low-luminosity collapsar event with a broad-line Type Ic supernova, supporting XRFs as the faint end of the long GRB population observed on-axis by a weak jet.
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Exploring Jet Structure and Dynamics in Short Gamma Ray Bursts: A Case Study on GRB 090510
GRMHD simulations of GRB 090510 predict energetics and jet opening angles consistent with observations within 1 sigma when jet angles evolve with redshift, while dynamical ejecta influence collimation and a suite of models explores broader GRB properties.
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Multi-wavelength study of EP250416a / GRB 250416C: An Optically Dark Long GRB with a Late Jet Break
EP250416a is an X-ray-rich long GRB at z=0.963 showing a late jet break at 1.5e6 s and optical darkness explained by A_V^host = 5.5 mag extinction.