Fig. 1.

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SFR vs. stellar mass of our full galaxy sample. Sources at 5.5 < z < 7.5 with new and archival C III] data, galaxies at z ∼ 2 with archival C III] data, and literature sample at 6.0 < z < 7.5 are shown as blue, green, and orange circles, respectively. The best-fit relations for the main sequence (MS) at 5.5 < z < 7.5 and 1.7 < z < 2.0 from Schreiber et al. (2015) are shown as magenta and red bands, respectively. SFR and stellar mass references: HZ1, HZ10 – Capak et al. (2015); RXJ 1347−1216 – Huang et al. (2016), Bradač et al. (2017); GDS3073 – Grazian et al. (2020); UVISTA-Z-002 – Bowler et al. (2017a), Bouwens et al. (2022); COS-3018 – Smit et al. (2018); A383-5.2 – Matthee et al. (2019), Stark et al. (2015); z7_GND_42912 – Schaerer et al. (2015); Himiko – Carniani et al. (2018b), Graziani et al. (2020); CR7, CR7a, CR7b, CR7c – Matthee et al. (2017a); Bowler et al. (2014, 2017b); COS-13679 – Matthee et al. (2019), Laporte et al. (2017); COS-2987 – Smit et al. (2018), Laporte et al. (2017); VR7 – Matthee et al. (2019, 2017b); 9347, 6515, 10076, 9834, 9681, 8490 – this work, Zanella et al. (2018).
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