Transverse clues on the kiloparsec-scale structure of the circumgalactic medium as traced by C IV absorption

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Fig. F.2.

Per-system 1-σ width of ξ^arc(Δv) displayed in Fig. 6. This is computed via a single Gaussian fit of ξ^arc(Δv) (x-axis) or predicted by the kinematic model described by Eq. (8), using σ₀ and N in Table 4 (y-axis). Error bars represent fit and propagated errors, respectively.

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