ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions

Mullaney, J.R., Alexander, D.M., Aird, J. et al. (15 more authors) (2015) ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions. (Submitted)

Abstract

Metadata

Authors/Creators:
  • Mullaney, J.R.
  • Alexander, D.M.
  • Aird, J.
  • Bernhard, E.
  • Daddi, E.
  • Moro, A.D.
  • Dickinson, M.
  • Elbaz, D.
  • Harrison, C.M.
  • Juneau, S.
  • Liu, D.
  • Pannella, M.
  • Rosario, D.
  • Santini, P.
  • Sargent, M.
  • Schreiber, C.
  • Simpson, J.
  • Stanley, F.
Keywords: astro-ph.GA; astro-ph.GA
Dates:
  • Published: 17 June 2015
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 30 Jun 2015 10:10
Last Modified: 29 Mar 2018 00:51
Status: Submitted
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