SN 2023aeaf is photometrically classified as a likely Type II supernova at z=3.195, consistent with a 12 solar mass progenitor and low-metallicity star-forming host.
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Statistical correlation analysis links the KM3-230213A neutrino to multiple GRBs within angular errors and computes LV scales incorporating redshift and energy uncertainties.
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Discovery and Analysis of a Type II Supernova Candidate at z = 3.19 from JWST's COSMOS-Web Survey
SN 2023aeaf is photometrically classified as a likely Type II supernova at z=3.195, consistent with a 12 solar mass progenitor and low-metallicity star-forming host.
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Correlation between Ultrahigh-Energy Neutrino KM3-230213A and Gamma-Ray Bursts
Statistical correlation analysis links the KM3-230213A neutrino to multiple GRBs within angular errors and computes LV scales incorporating redshift and energy uncertainties.