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Fig. 9


Left panel: relative differences in right ascension and declination between object coordinates in the MUSE-Wide catalogue and objects with the closest on-sky separation in the 3D-HST catalogue (Skelton et al. 2014). Right panel: angular separation Δρ for between MUSE-Wide objects and most closely separated 3D-HST sources. 83% of the objects from our MUSE-Wide catalogue have cross-matches within 0.5′′ in the Skelton et al. (2014) catalogue.

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