Table 3.

Median sizes and total magnitudes in the rest-frame UV and optical of the subsamples divided into three redshift bins.*

RedshiftFlagMUVreMoptre, opt
(mag)(kpc)(mag)(kpc)
(1)(2)(3)(4)(5)(6)
z = 4.5–5.51−19.89|$0.36^{+0.17}_{-0.11}$|−20.58|$0.47^{+0.30}_{-0.15}$|
2−19.83|$0.41^{+0.22}_{-0.15}$|−20.35|$0.49^{+0.21}_{-0.15}$|
2−20.30|$0.55^{+0.27}_{-0.27}$|−20.89|$0.59^{+0.23}_{-0.17}$|
2−20.95|$0.77^{+0.44}_{-0.41}$|−21.72|$0.89^{+0.41}_{-0.39}$|
z = 5.5–6.51−19.96|$0.40^{+0.09}_{-0.19}$|−21.45|$0.36^{+0.29}_{-0.13}$|
2−20.10|$0.41^{+0.13}_{-0.22}$|−20.92|$0.56^{+0.23}_{-0.26}$|
2−20.69|$0.76^{+0.10}_{-0.39}$|−22.20|$0.75^{+0.22}_{-0.16}$|
z = 6.5–9.51−20.27|$0.13^{+0.10}_{-0.05}$|−20.75|$0.24^{+0.04}_{-0.05}$|
2−20.05|$0.22^{+0.11}_{-0.12}$|−20.70|$0.28^{+0.24}_{-0.06}$|
2−20.73|$0.20^{+0.32}_{-0.05}$|−21.63|$0.26^{+0.19}_{-0.11}$|
RedshiftFlagMUVreMoptre, opt
(mag)(kpc)(mag)(kpc)
(1)(2)(3)(4)(5)(6)
z = 4.5–5.51−19.89|$0.36^{+0.17}_{-0.11}$|−20.58|$0.47^{+0.30}_{-0.15}$|
2−19.83|$0.41^{+0.22}_{-0.15}$|−20.35|$0.49^{+0.21}_{-0.15}$|
2−20.30|$0.55^{+0.27}_{-0.27}$|−20.89|$0.59^{+0.23}_{-0.17}$|
2−20.95|$0.77^{+0.44}_{-0.41}$|−21.72|$0.89^{+0.41}_{-0.39}$|
z = 5.5–6.51−19.96|$0.40^{+0.09}_{-0.19}$|−21.45|$0.36^{+0.29}_{-0.13}$|
2−20.10|$0.41^{+0.13}_{-0.22}$|−20.92|$0.56^{+0.23}_{-0.26}$|
2−20.69|$0.76^{+0.10}_{-0.39}$|−22.20|$0.75^{+0.22}_{-0.16}$|
z = 6.5–9.51−20.27|$0.13^{+0.10}_{-0.05}$|−20.75|$0.24^{+0.04}_{-0.05}$|
2−20.05|$0.22^{+0.11}_{-0.12}$|−20.70|$0.28^{+0.24}_{-0.06}$|
2−20.73|$0.20^{+0.32}_{-0.05}$|−21.63|$0.26^{+0.19}_{-0.11}$|

*(1) Redshift range. (2) Flag for spectroscopic redshifts: 1. galaxies with spectroscopic confirmation; 2. galaxies with and without spectroscopic confirmation. (3) Median rest-frame UV total magnitude. (4) Median size in the rest-frame UV and its 68th percentiles. (5) Median rest-frame optical total magnitude. (6) Median size in the rest-frame optical and its 68th percentiles.

Table 3.

Median sizes and total magnitudes in the rest-frame UV and optical of the subsamples divided into three redshift bins.*

RedshiftFlagMUVreMoptre, opt
(mag)(kpc)(mag)(kpc)
(1)(2)(3)(4)(5)(6)
z = 4.5–5.51−19.89|$0.36^{+0.17}_{-0.11}$|−20.58|$0.47^{+0.30}_{-0.15}$|
2−19.83|$0.41^{+0.22}_{-0.15}$|−20.35|$0.49^{+0.21}_{-0.15}$|
2−20.30|$0.55^{+0.27}_{-0.27}$|−20.89|$0.59^{+0.23}_{-0.17}$|
2−20.95|$0.77^{+0.44}_{-0.41}$|−21.72|$0.89^{+0.41}_{-0.39}$|
z = 5.5–6.51−19.96|$0.40^{+0.09}_{-0.19}$|−21.45|$0.36^{+0.29}_{-0.13}$|
2−20.10|$0.41^{+0.13}_{-0.22}$|−20.92|$0.56^{+0.23}_{-0.26}$|
2−20.69|$0.76^{+0.10}_{-0.39}$|−22.20|$0.75^{+0.22}_{-0.16}$|
z = 6.5–9.51−20.27|$0.13^{+0.10}_{-0.05}$|−20.75|$0.24^{+0.04}_{-0.05}$|
2−20.05|$0.22^{+0.11}_{-0.12}$|−20.70|$0.28^{+0.24}_{-0.06}$|
2−20.73|$0.20^{+0.32}_{-0.05}$|−21.63|$0.26^{+0.19}_{-0.11}$|
RedshiftFlagMUVreMoptre, opt
(mag)(kpc)(mag)(kpc)
(1)(2)(3)(4)(5)(6)
z = 4.5–5.51−19.89|$0.36^{+0.17}_{-0.11}$|−20.58|$0.47^{+0.30}_{-0.15}$|
2−19.83|$0.41^{+0.22}_{-0.15}$|−20.35|$0.49^{+0.21}_{-0.15}$|
2−20.30|$0.55^{+0.27}_{-0.27}$|−20.89|$0.59^{+0.23}_{-0.17}$|
2−20.95|$0.77^{+0.44}_{-0.41}$|−21.72|$0.89^{+0.41}_{-0.39}$|
z = 5.5–6.51−19.96|$0.40^{+0.09}_{-0.19}$|−21.45|$0.36^{+0.29}_{-0.13}$|
2−20.10|$0.41^{+0.13}_{-0.22}$|−20.92|$0.56^{+0.23}_{-0.26}$|
2−20.69|$0.76^{+0.10}_{-0.39}$|−22.20|$0.75^{+0.22}_{-0.16}$|
z = 6.5–9.51−20.27|$0.13^{+0.10}_{-0.05}$|−20.75|$0.24^{+0.04}_{-0.05}$|
2−20.05|$0.22^{+0.11}_{-0.12}$|−20.70|$0.28^{+0.24}_{-0.06}$|
2−20.73|$0.20^{+0.32}_{-0.05}$|−21.63|$0.26^{+0.19}_{-0.11}$|

*(1) Redshift range. (2) Flag for spectroscopic redshifts: 1. galaxies with spectroscopic confirmation; 2. galaxies with and without spectroscopic confirmation. (3) Median rest-frame UV total magnitude. (4) Median size in the rest-frame UV and its 68th percentiles. (5) Median rest-frame optical total magnitude. (6) Median size in the rest-frame optical and its 68th percentiles.

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