Fig. 5.

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Mass discrepancy between the integrated cases and the resolved CSFH, as a function of the unresolved specific star formation rate. The dashed line indicates no offset (or ratio = 1). The purple points correspond to spectroscopically confirmed galaxies at 0 < z < 2.5 from Sorba & Sawicki (2018) (using an exponentially declining SFH). The turquoise diamonds are 5 < z < 9 galaxies from Giménez-Arteaga et al. (2023) (using a CSFH). The square and stars correspond to this work. The black square indicates the fiducial CSFH case. The red, orange and blue stars indicate a double-power law, a log-normal, and an exponentially declining SFH parameterisations, respectively.
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