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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2026 2representative citing papers
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.
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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A new wideband radio polarization observation of the Supernova Remnant G315.4$-$2.3
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.