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

Mullaney, J. R., Alexander, D. M., Aird, J., Bernhard, E., Daddi, E., Moro, A. D., et al. (2015). ALMA and Herschel reveal that X-ray-selected AGN and main-sequence galaxies have different star formation rate distributions. Monthly Notices of the Royal Astronomical Society: Letters, 453(1), L83-L87. doi:10.1093/mnrasl/slv110.

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 Creators:
Mullaney, J. R., Author
Alexander, D. M., Author
Aird, J., Author
Bernhard, E., Author
Daddi, E., Author
Moro, A. Del, Author
Dickinson, M., Author
Elbaz, D., Author
Harrison, C. M., Author
Juneau, S., Author
Liu, D., Author
Pannella, M., Author
Rosario, D.1, Author           
Santini, P., Author
Sargent, M., Author
Schreiber, C., Author
Simpson, J., Author
Stanley, F., Author
Affiliations:
1Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159889              

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Language(s): -
 Dates: 2015-10-11
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnrasl/slv110
Other: LOCALID: 2223785
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Title: Monthly Notices of the Royal Astronomical Society: Letters
  Alternative Title : Mon. Not. Roy. Astron. Soc.: Letters
Source Genre: Journal
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Pages: 5 Volume / Issue: 453 (1) Sequence Number: - Start / End Page: L83 - L87 Identifier: ISSN: 1364-8711
ISSN: 0035-8711