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Phibss: molecular gas content and scaling relations in z ~ 1-3 massive, main-sequence star-forming galaxies

MPS-Authors
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Tacconi,  L. J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Wuyts,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Gracia-Carpio,  J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Naab,  T.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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

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Citation

Tacconi, L. J., Neri, R., Genzel, R., Combes, F., Bolatto, A., Cooper, M. C., et al. (2013). Phibss: molecular gas content and scaling relations in z ~ 1-3 massive, main-sequence star-forming galaxies. The Astrophysical Journal, 768(1): 74, pp. 1-22. doi:10.1088/0004-637X/768/1/74.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0013-ACE8-A
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