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Fig. 1

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Location of the lines of sight in the LMC. The total metallicities in the neutral ISM along these lines of sight are highlighted in greyscale. The systems with metallicities that are significantly lower than the nominal value (deviating by 3σ) are highlighted in orange. The metallicities of other lines of sight are consistent with the nominal value for hot stars, within the uncertainties. The background image is from DSS2.

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