Figure 2 (IMAGE)

Kavli Institute for the Physics and Mathematics of the Universe

Figure 2

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Figure 2: Size–luminosity relationships of galaxies observed in five wavelength bands with fixed slope owing to limited data. The black solid and dashed–dotted lines in the F150W panel show the relation derived from HST data by Shibuya et al. (2015; z ∼ 8) and Huang et al. (2013; z ∼ 5) at a similar rest-frame wavelength, respectively.

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Yang et al.

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