Extended Data Table 1 Physical properties of the 17 galaxy-size clumps and the entire JQ system

From: Extended enriched gas in a multi-galaxy merger at redshift 6.7

  1. The physical properties of clumps are obtained from fitting the SEDs of individual clumps, while the total stellar mass and SFR of JQ are determined through a spatially resolved analysis of the entire JQ system. The total [O III]+Hβ luminosity is derived by summing the [O III]+Hβ map. See Methods for details about the SED fitting.
Back to article page