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The evolution of the mass function split by morphology up to redshift 1 in the FORS deep and the GOODS-S fields

MPS-Authors
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Pannella,  M.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Hopp,  U.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Saglia,  R. P.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Bender,  R.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Feulner,  G.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Pannella, M., Hopp, U., Saglia, R. P., Bender, R., Drory, N., Salvato, M., et al. (2006). The evolution of the mass function split by morphology up to redshift 1 in the FORS deep and the GOODS-S fields. The Astrophysical Journal, 639(1 Part 2), L1-L4. doi:10.1086/501452.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-D510-9
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