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Fig. 5.

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Intensity and polarisation maps around the W43 molecular cloud. The three rows show, respectively, I, Q, and U maps, while the columns correspond to QUIJOTE-MFI 17 (Horn 2) and 19 GHz (Horn 2) and to WMAP 23 GHz, from left to right. The solid circle shows the aperture we used for flux integration, whereas the two dashed circles enclose the ring we used for background subtraction.

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