On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8

Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot, Hans Walter Rix, Mattia Fumagalli, Arjen van der Wel, Marijn Franx, Michael V. Maseda, Pieter G. Van Dokkum, Gabriel B. Brammer, Ivelina Momcheva, Rosalind E. Skelton, Katherine Whitaker, Joel Leja, Britt Lundgren, Susan A. Kassin, Sukyoung K. Yi

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