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This article has an erratum: [https://doi.org/10.1051/0004-6361/202038904e]


Fig. 6.

image

Location of the CL1411 (grey) and ALMA (green) galaxies in the stellar mass–SFR plane. The dots with thick black borders represent the Spitzer-observed galaxies and those with the pink outline indicate the low-μH2 galaxies. Galaxies in black and grey are the rest of the spectroscopic and photometric samples, respectively, at the cluster redshift. The plain orange circles are the PHIBSS2 galaxies with 0.49 ≤ z ≤ 0.6, while the light orange circles trace the PHIBSS2 sample at 0.6 < z ≤ 0.8; the orange squares show the cluster LIRGs of Castignani et al. (2020) at z ∼ 0.54. The dashed black line is the Speagle et al. (2014) MS corrected for a Chabrier IMF, at our cluster redshift with the corresponding ±0.3 dex scatter as the grey shaded area.

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