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Fig. 1


SN2014J spectrum near the 847 keV line (above) and near the 1238 keV line (below) as expected from 56Co decay. These spectra are determined in energy bins of width 10 keV over the entire observing period; the source intensity is fitted at four independent epochs. For illustration, fitted Gaussians indicate the detection of broadened lines near the 56Co gamma-ray line energies.

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