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

Pannella, M.; Hopp, U.; Saglia, R. P.; Bender, R.; Drory, N.; Salvato, M.; Feulner, G.

doi:10.1086/501452

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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

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

/persons/resource/persons4757

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

/persons/resource/persons18398

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

/persons/resource/persons4759

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;

/persons/resource/persons23049

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

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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: https://hdl.handle.net/11858/00-001M-0000-0011-D510-9

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