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Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1

MPS-Authors
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Wuyts,  Stijn
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Förster Schreiber,  Natascha M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Magnelli,  Benjamin
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Genzel,  Reinhard
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lutz,  Dieter
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Berta,  Stefano
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Graciá-Carpio,  Javier
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Saintonge,  Amelie
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Tacconi,  Linda
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Wuyts, S., Förster Schreiber, N. M., van der Wel, A., Magnelli, B., Guo, Y., Genzel, R., et al. (2011). Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1. The Astrophysical Journal, 742(2): 96, pp. 1-20. doi:10.1088/0004-637X/742/2/96.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-3A2B-A
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