PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z ≤ 2.5

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Table 3.

Physical properties of galaxies in the three categories.

Category(#)	z	log(M_*/M_⊙)	SFR/M_⊙ yr⁻¹	ΔMS	$n_{optical}^{corrected}$ $n_{\text{ optical}}^{\text{ corrected}}$	n_MIR	$R e_{optical}^{corrected} /$ $Re_{\text{ optical}}^{\text{ corrected}}/$ kpc	Re_MIR/kpc	$b / a_{optical}^{corrected}$ $b/a_{\text{ optical}}^{\text{ corrected}}$	b/a_MIR
CC(74)	$1 . 19_{- 0.56}^{+ 0.51}$ $1.19_{-0.56}^{+0.51}$	$10 . 04_{- 0.31}^{+ 0.44}$ $10.04_{-0.31}^{+0.44}$	$17 . 11_{- 11.11}^{+ 41.69}$ $17.11_{-11.11}^{+41.69}$	$0 . 16_{- 0.24}^{+ 0.16}$ $0.16_{-0.24}^{+0.16}$	$1 . 35_{- 0.55}^{+ 1.31}$ $1.35_{-0.55}^{+1.31}$	$0 . 77_{- 0.36}^{+ 0.46}$ $0.77_{-0.36}^{+0.46}$	$1 . 66_{- 0.34}^{+ 0.41}$ $1.66_{-0.34}^{+0.41}$	$1 . 8_{- 0.43}^{+ 0.59}$ $1.8_{-0.43}^{+0.59}$	$0 . 74_{- 0.22}^{+ 0.13}$ $0.74_{-0.22}^{+0.13}$	$0 . 78_{- 0.16}^{+ 0.09}$ $0.78_{-0.16}^{+0.09}$
EE(254)	$1 . 15_{- 0.51}^{+ 0.45}$ $1.15_{-0.51}^{+0.45}$	$10 . 1_{- 0.3}^{+ 0.37}$ $10.1_{-0.3}^{+0.37}$	$17 . 28_{- 11.29}^{+ 44.49}$ $17.28_{-11.29}^{+44.49}$	$0 . 11_{- 0.2}^{+ 0.21}$ $0.11_{-0.2}^{+0.21}$	$0 . 91_{- 0.35}^{+ 0.7}$ $0.91_{-0.35}^{+0.7}$	$0 . 64_{- 0.22}^{+ 0.47}$ $0.64_{-0.22}^{+0.47}$	$3 . 73_{- 1.1}^{+ 1.56}$ $3.73_{-1.1}^{+1.56}$	$3 . 5_{- 0.93}^{+ 1.7}$ $3.5_{-0.93}^{+1.7}$	$0 . 51_{- 0.21}^{+ 0.28}$ $0.51_{-0.21}^{+0.28}$	$0 . 56_{- 0.19}^{+ 0.24}$ $0.56_{-0.19}^{+0.24}$
EC(56)	$1 . 38_{- 0.69}^{+ 0.52}$ $1.38_{-0.69}^{+0.52}$	$10 . 35_{- 0.46}^{+ 0.45}$ $10.35_{-0.46}^{+0.45}$	$31 . 56_{- 23.97}^{+ 106.38}$ $31.56_{-23.97}^{+106.38}$	$0 . 2_{- 0.28}^{+ 0.21}$ $0.2_{-0.28}^{+0.21}$	$1 . 42_{- 0.73}^{+ 1.58}$ $1.42_{-0.73}^{+1.58}$	$1 . 23_{- 0.54}^{+ 0.73}$ $1.23_{-0.54}^{+0.73}$	$4 . 04_{- 1.04}^{+ 1.86}$ $4.04_{-1.04}^{+1.86}$	$2 . 13_{- 0.97}^{+ 0.94}$ $2.13_{-0.97}^{+0.94}$	$0 . 49_{- 0.18}^{+ 0.27}$ $0.49_{-0.18}^{+0.27}$	$0 . 64_{- 0.18}^{+ 0.18}$ $0.64_{-0.18}^{+0.18}$
CC^*(58)	$1 . 2_{- 0.46}^{+ 0.32}$ $1.2_{-0.46}^{+0.32}$	$10 . 05_{- 0.24}^{+ 0.41}$ $10.05_{-0.24}^{+0.41}$	$18 . 17_{- 8.88}^{+ 23.45}$ $18.17_{-8.88}^{+23.45}$	$0 . 16_{- 0.23}^{+ 0.15}$ $0.16_{-0.23}^{+0.15}$	$1 . 47_{- 0.65}^{+ 1.23}$ $1.47_{-0.65}^{+1.23}$	$0 . 85_{- 0.34}^{+ 0.4}$ $0.85_{-0.34}^{+0.4}$	$1 . 66_{- 0.33}^{+ 0.44}$ $1.66_{-0.33}^{+0.44}$	$1 . 85_{- 0.49}^{+ 0.54}$ $1.85_{-0.49}^{+0.54}$	$0 . 76_{- 0.17}^{+ 0.11}$ $0.76_{-0.17}^{+0.11}$	$0 . 8_{- 0.15}^{+ 0.08}$ $0.8_{-0.15}^{+0.08}$
EE^*(211)	$1 . 18_{- 0.5}^{+ 0.4}$ $1.18_{-0.5}^{+0.4}$	$10 . 09_{- 0.23}^{+ 0.32}$ $10.09_{-0.23}^{+0.32}$	$17 . 39_{- 9.33}^{+ 28.67}$ $17.39_{-9.33}^{+28.67}$	$0 . 11_{- 0.2}^{+ 0.2}$ $0.11_{-0.2}^{+0.2}$	$0 . 88_{- 0.32}^{+ 0.7}$ $0.88_{-0.32}^{+0.7}$	$0 . 64_{- 0.22}^{+ 0.38}$ $0.64_{-0.22}^{+0.38}$	$3 . 73_{- 1.1}^{+ 1.54}$ $3.73_{-1.1}^{+1.54}$	$3 . 59_{- 0.98}^{+ 1.51}$ $3.59_{-0.98}^{+1.51}$	$0 . 5_{- 0.18}^{+ 0.29}$ $0.5_{-0.18}^{+0.29}$	$0 . 57_{- 0.2}^{+ 0.22}$ $0.57_{-0.2}^{+0.22}$
EC^*(38)	$1 . 24_{- 0.53}^{+ 0.48}$ $1.24_{-0.53}^{+0.48}$	$10 . 24_{- 0.34}^{+ 0.31}$ $10.24_{-0.34}^{+0.31}$	$24 . 78_{- 14.56}^{+ 43.77}$ $24.78_{-14.56}^{+43.77}$	$0 . 1_{- 0.26}^{+ 0.25}$ $0.1_{-0.26}^{+0.25}$	$1 . 41_{- 0.76}^{+ 1.32}$ $1.41_{-0.76}^{+1.32}$	$1 . 25_{- 0.46}^{+ 0.51}$ $1.25_{-0.46}^{+0.51}$	$4 . 21_{- 1.16}^{+ 1.71}$ $4.21_{-1.16}^{+1.71}$	$2 . 23_{- 0.83}^{+ 0.84}$ $2.23_{-0.83}^{+0.84}$	$0 . 48_{- 0.17}^{+ 0.23}$ $0.48_{-0.17}^{+0.23}$	$0 . 59_{- 0.14}^{+ 0.21}$ $0.59_{-0.14}^{+0.21}$

Notes. Median values of physical properties for galaxies in the three categories defined in Fig. 14. Upper and lower ranges are derived from the 16th and 84th percentiles. For those labeled with “*,” the sample is limited to 10^9.7 < (M_*/M_⊙) < 10^10.7 and z < 2.

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