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A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34

The author's prominent role in this paper is recognised by his position as third author, in the group of major contributors behind the project leader as first author. He contributed significantly to the conception, design, organisation and conduct of this study. Specific areas include independent confirmation of the initial source selection, acquiring and analysing follow-up data from the Submillimetre Array Telescope, contributing to the continuum SED analysis, and in comparisons to other high redshift populations. The author also contributed to drafting the paper and accompanying supplementary material.