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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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.HE 2representative citing papers
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.
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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The Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.