Extended Data Fig. 7: Results from triaxial modelling for the subsamples of galaxies split by flux density and beam size.
From: In situ spheroid formation in distant submillimetre-bright galaxies
The median flux density at band 7 and the median beam size for the full sample are \({7.8}_{-4.7}^{+3.6}\,{\rm{mJy}}\) and \(0.5{1}_{-0.31}^{+0.39}\,{\rm{arcsec}}\) (uncertainties are interquartile range), respectively. a,b, A subsample of galaxies with flux brighter than the median value. The ⟨B/A⟩ and ⟨C/A⟩ are 0.88 ± 0.06 and 0.50 ± 0.04, respectively. c,d, A subsample of galaxies with flux fainter than the median value. The ⟨B/A⟩ and ⟨C/A⟩ are 0.89 ± 0.07 and 0.51 ± 0.05, respectively. e,f, A subsample of galaxies with beam size larger than the median value. The ⟨B/A⟩ and ⟨C/A⟩ are 0.87 ± 0.07 and 0.49 ± 0.04, respectively. g,h, A subsample of galaxies with beam size smaller than the median value. The ⟨B/A⟩ and ⟨C/A⟩ are 0.90 ± 0.06 and 0.52 ± 0.04, respectively.
