Fig. 7.
(Left) Comparison of stellar masses obtained by MAGPHYS and FAST. The black dashed line indicates the case that log (M*/$M_\odot$)MAGPHYS = log (M*/$M_\odot$)FAST. (Right) Comparison of IR + UV SFRs obtained by MAGPHYS and ZFOURGE. The black dashed line indicates the case that $\log (\mathit {SFR}_\mathrm{UV+IR})_\mathrm{MAGPHYS} = \log (\mathit {SFR}_\mathrm{UV+IR})_\mathrm{ZFOURGE}$.

(Left) Comparison of stellar masses obtained by MAGPHYS and FAST. The black dashed line indicates the case that log (M*/|$M_\odot$|⁠)MAGPHYS = log (M*/|$M_\odot$|⁠)FAST. (Right) Comparison of IR + UV SFRs obtained by MAGPHYS and ZFOURGE. The black dashed line indicates the case that |$\log (\mathit {SFR}_\mathrm{UV+IR})_\mathrm{MAGPHYS} = \log (\mathit {SFR}_\mathrm{UV+IR})_\mathrm{ZFOURGE}$|⁠.

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