The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day
C. Schreiber, M. Pannella, D. Elbaz, M. Béthermin, H. Inami, M. Dickinson, B. Magnelli, T. Wang, H. Aussel, E. Daddi, S. Juneau, X. Shu, M. T. Sargent, V. Buat, S. M. Faber, H. C. Ferguson, M. Giavalisco, A. M. Koekemoer, G. Magdis, G. E. Morrison, C. Papovich, P. Santini and D. Scott
A&A, 575 (2015) A74
DOI: https://doi.org/10.1051/0004-6361/201425017
