Uncertainties in high-z galaxy properties inferred from spectral energy distribution fittings using JWST NIRCam photometry

Open Access

Fig. 10.

Same as Fig. 5, but for the attS_Z model adopting an SMC-type dust attenuation curve. Compared to Fig. 5, the underestimation of SFR₁₀ is apparent across the entire stellar-mass range, while the underestimation of SFR₁₀₀ becomes progressively more severe toward the high-mass end.

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