- Arango-Toro, RC;
- Ilbert, O;
- Ciesla, L;
- Shuntov, M;
- Aufort, G;
- Mercier, W;
- Laigle, C;
- Franco, M;
- Bethermin, M;
- Le Borgne, D;
- Dubois, Y;
- McCracken, HJ;
- Paquereau, L;
- Huertas-Company, M;
- Kartaltepe, J;
- Casey, CM;
- Akins, H;
- Allen, N;
- Andika, I;
- Brinch, M;
- Drakos, NE;
- Faisst, A;
- Gozaliasl, G;
- Harish, S;
- Kaminsky, A;
- Koekemoer, A;
- Kokorev, V;
- Liu, D;
- Magdis, G;
- Martin, CL;
- Moutard, T;
- Rhodes, J;
- Rich, RM;
- Robertson, B;
- Sanders, DB;
- Sheth, K;
- Talia, M;
- Toft, S;
- Tresse, L;
- Valentino, F;
- Vijayan, A;
- Weaver, J
Context. The stellar mass-star formation rate (M-a a a SFR) plane is an essential diagnostic to separate galaxy populations. However, we still lack a clear picture of how galaxies move within this plane along cosmic time. Aims. This study aims to provide an observational description of galaxy migrations in the M-a a a SFR plane based on the reconstructed star formation histories (SFH) of a sample of galaxies at redshift za
