ALMA Detection of Extended [CII] Emission in Himiko at z=6.6

Himiko is one of the most luminous Lyα emitters at z = 6.595. It has three star-forming clumps detected in the rest-frame UV, with a total SFR = 20 M ⊙ yr−1. We report the Atacama Large Millimeter/submillimeter Array (ALMA) detection of the [C ii]158 μm line emission in this Galaxy with a significance of 8σ. The total [C ii] luminosity (L [C ii] = 1.2 × 108 L ⊙) is fully consistent with the local L [C ii]–SFR relation. The ALMA high-angular resolution reveals that the [C ii] emission is made of two distinct components. The brightest [C ii] clump is extended over 4 kpc and is located on the peak of the Lyα nebula, which is spatially offset by 1 kpc relative to the brightest UV clump. The second [C ii] component is spatially unresolved (size