Transition from outside-in to inside-out at z ∼ 2: Evidence from radial profiles of the specific star formation rate based on JWST/HST

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Table 1.

sSFR gradient at different stellar masses and redshift bins.

sSFR gradient between 0.5R_e and 2.5R_e in unit of dex/R_e
	0 < z < 0.5	0.5 < z < 1	1 < z < 1.5	1.5 < z < 2	2 < z < 2.5	2.5 < z < 3	3 < z < 3.5	3.5 < z < 4

8 < log(M_*/M_⊙) < 9	0.083 ± 0.010	0.101 ± 0.003	0.096 ± 0.003	0.078 ± 0.002	−0.003 ± 0.004	−0.051 ± 0.005	−0.064 ± 0.006	−0.046 ± 0.006
9 < log(M_*/M_⊙) < 10	0.001 ± 0.002	0.029 ± 0.006	0.050 ± 0.004	0.055 ± 0.004	−0.003 ± 0.004	−0.034 ± 0.005	−0.049 ± 0.006	−0.035 ± 0.005
10 < log(M_*/M_⊙) < 12	0.115 ± 0.005	0.144 ± 0.017	0.184 ± 0.015	0.080 ± 0.015	0.058 ± 0.019	−0.071 ± 0.025	−0.030 ± 0.034	−0.037 ± 0.038

sSFR gradient between 0.5 Kpc and 2.5 Kpc in unit of dex/kpc

	0 < z < 0.5	0.5 < z < 1	1 < z < 1.5	1.5 < z < 2	2 < z < 2.5	2.5 < z < 3	3 < z < 3.5	3.5 < z < 4

8 < log(M_*/M_⊙) < 9	0.041 ± 0.008	0.031 ± 0.003	0.035 ± 0.003	0.023 ± 0.002	−0.004 ± 0.004	−0.022 ± 0.005	−0.021 ± 0.005	−0.039 ± 0.006
9 < log(M_*/M_⊙) < 10	0.045 ± 0.019	0.021 ± 0.006	0.006 ± 0.004	0.002 ± 0.003	−0.017 ± 0.004	−0.022 ± 0.004	−0.025 ± 0.005	−0.041 ± 0.005
10 < log(M_*/M_⊙) < 12	0.157 ± 0.045	0.216 ± 0.016	0.194 ± 0.017	0.098 ± 0.018	0.067 ± 0.020	−0.010 ± 0.031	0.025 ± 0.033	−0.013 ± 0.029

sSFR gradient derived from deconvolved images between 0.5 Kpc and 2.5 Kpc in unit of dex/kpc

8 < log(M_*/M_⊙) < 9	0.064 ± 0.009	0.057 ± 0.004	0.065 ± 0.004	0.061 ± 0.004	−0.034 ± 0.005	−0.063 ± 0.006	−0.064 ± 0.007	−0.046 ± 0.009
9 < log(M_*/M_⊙) < 10	0.082 ± 0.020	0.044 ± 0.007	0.018 ± 0.006	−0.012 ± 0.005	−0.056 ± 0.005	−0.072 ± 0.006	−0.059 ± 0.009	−0.090 ± 0.008
10 < log(M_*/M_⊙) < 12	0.338 ± 0.050	0.304 ± 0.019	0.311 ± 0.023	0.186 ± 0.027	0.137 ± 0.028	0.011 ± 0.031	0.060 ± 0.046	−0.013 ± 0.060

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