Fig. 9.
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Spectra of the three filaments detected in the high-resolution images. We have added two best-fit power laws for filaments F1 and F3; the spectrum of filament F2 is not consistent with a power law due to the spectral steepening. For this reason, we have measured the spectral index by linking the three flux density values. The legend is shown in the bottom-left corner along with the spectral index value.
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