Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference

Open Access

Fig. 11.

Number of maxima 〈m〉 in the COSMOS (top) and Horizon-AGN (bottom) SFHs as a function of stellar mass, colour-coded by the formation look-back time for two different redshift bins. The number of maxima is computed as described in Section 4.2.3 and Fig. 9.

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