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

dc.creator	Schreiber, C.
dc.creator	Pannella, M.
dc.creator	Elbaz, D.
dc.creator	Béthermin, M.
dc.creator	Inami, H.
dc.creator	Dickinson, M.
dc.creator	Magnelli, B.
dc.creator	Wang, T.
dc.creator	Aussel, H.
dc.creator	Daddi, E.
dc.creator	Juneau, S.
dc.creator	Shu, X.
dc.creator	Sargent, M. T.
dc.creator	Buat, V.
dc.creator	Faber, S. M.
dc.creator	Ferguson, H. C.
dc.creator	Giavalisco, M.
dc.creator	Koekemoer, A. M.
dc.creator	Magdis, G.
dc.creator	Morrison, G. E.
dc.creator	Papovich, C.
dc.creator	Santini, P.
dc.creator	Scott, D.
dc.date.accessioned	2019-10-09T16:21:49Z
dc.date.available	2019-10-09T16:21:49Z
dc.date.issued	2015
dc.identifier.issn	0004-6361
dc.identifier.issn	1432-0746
dc.identifier.uri	https://hdl.handle.net/1969.1/180624
dc.format.extent	1	en
dc.publisher	Astronomy and Astrophysics
dc.relation.ispartof	1foldr Import 2019-10-08 Batch 5	en
dc.relation.uri	10.1051/0004-6361/201425017	en
dc.title	The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day	en