Skip to main content
Unpublished Paper
The Herschel View of the Dominant Mode of Galaxy Growth From z=4 to the Present Day
Astronomy & Astrophysics (2015)
  • C. Schreiber
  • M. Pannella
  • D. Elbaz
  • M. Bethermin
  • 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
  • Mauro Giavalisco, University of Massachusetts - Amherst
  • A.M. Koekemoer
  • G. Magdis
  • G.E. Morrison
  • C. Papovich
  • P. Santini
  • D. Scott
Keywords
  • Galaxies: evolution,
  • Galaxies: active,
  • Galaxies: starburst,
  • Infrared: galaxies,
  • Methods: statistical
Publication Date
2015
Comments
Prepublished version downloaded from ArXiv. Published version is located at http://www.aanda.org/articles/aa/abs/2015/03/aa25017-14/aa25017-14.html
Citation Information
C. Schreiber, M. Pannella, D. Elbaz, M. Bethermin, et al.. "The Herschel View of the Dominant Mode of Galaxy Growth From z=4 to the Present Day" Astronomy & Astrophysics (2015)
Available at: http://works.bepress.com/mauro_giavalisco/76/