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.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Larger-sample positional analysis of HI gas shows all SN types deviate from random but are mutually consistent and not linked to densest atomic gas concentrations unlike GRBs.
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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Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c
Larger-sample positional analysis of HI gas shows all SN types deviate from random but are mutually consistent and not linked to densest atomic gas concentrations unlike GRBs.