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The evolution of the star formation activity per halo mass up to redshift ~1.6 as seen by Herschel

MPS-Authors
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Popesso,  P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Salvato,  M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons16227

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

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Finoguenov,  A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons16221

Magnelli,  B.
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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Förster Schreiber,  N.
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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Nordon,  R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Shao,  L.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Citation

Popesso, P., Biviano, A., Rodighiero, G., Baronchelli, I., Salvato, M., Saintonge, A., et al. (2012). The evolution of the star formation activity per halo mass up to redshift ~1.6 as seen by Herschel. Astronomy & Astrophysics, 537: A58, pp. 1-8. doi:10.1051/0004-6361/201117973.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-873A-C
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