The Herschel view of the dominant mode of galaxy growth from z = 4 to the 
present day

Schreiber, C.; Pannella, M.; Elbaz, D.; Béthermin, M.; Inami, H.; Dickinson, M.; Magnelli, B.; Wang, T.; Aussel, H.; Daddi, E.; Juneau, S.; Shu, X.; Sargent, M. T.; Buat, V.; Faber, S. M.; Ferguson, H. C.; Giavalisco, M.; Koekemoer, A. M.; Magdis, G.; Morrison, G. E.; Papovich, C.; Santini, P.; Scott, D.

doi:10.1051/0004-6361/201425017

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The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day

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Magnelli, B.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Schreiber, C., Pannella, M., Elbaz, D., Béthermin, M., Inami, H., Dickinson, M., et al. (2015). The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day. Astronomy & Astrophysics, 575: A74, pp. 1-29. doi:10.1051/0004-6361/201425017.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0027-7ABA-A

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