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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In neutron star merger ejecta simulations, coupling in-situ nuclear networks with composition-dependent thermalization and frequency-dependent opacities changes nucleosynthesis yields, delays and reddens early emission, and produces brighter, bluer kilonovae than simplified analytic prescriptions.
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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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Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae
In neutron star merger ejecta simulations, coupling in-situ nuclear networks with composition-dependent thermalization and frequency-dependent opacities changes nucleosynthesis yields, delays and reddens early emission, and produces brighter, bluer kilonovae than simplified analytic prescriptions.