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. Del; 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.

doi:10.1093/mnrasl/slv110

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

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Rosario, D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0028-DDE5-A

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