Fitting spectral energy distributions of FMOS-COSMOS emission-line galaxies at z ∼ 1.6: Star formation rates, dust attenuation, and [OIII]λ5007 emission-line luminositiesJ. A. Villa-Vélez, V. Buat, P. Theulé, M. Boquien and D. BurgarellaA&A, 654 (2021) A153DOI: https://doi.org/10.1051/0004-6361/202140890
