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Fig. 1.

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MUSE arc images and C IV system maps. Columns from left to right: Column (1): White-image stamps of the gravitational arcs. Column (2): 0 . 6 × 0 . 6 $ 0{{\overset{\prime\prime}{.}}}6\times0{{\overset{\prime\prime}{.}}}6 $-binned spaxels with C IV detections, colored according to their significance (Sect. 3.2). Spaxel coordinates as in Figs. A.1–A.8. In both columns, the PSF is represented by the lower-right circle. Columns (3), (4), and (5): Absorber-plane reconstructed maps of equivalent width (W01548), velocity, and absorption spread, respectively. In all panels, the scale is indicated. In Columns (2)–(5), the triangles indicate W0 ≤ 0.2 Å (2-σ) non-detections.

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