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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

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.

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 Creators:
Pannella, M.1, Author           
Hopp, U.1, Author           
Saglia, R. P.1, Author           
Bender, R.1, Author           
Drory, N., Author
Salvato, M.2, Author           
Feulner, G.1, Author           
Affiliations:
1Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              
2High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2006-03-01
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: eDoc: 261147
DOI: 10.1086/501452
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Title: The Astrophysical Journal
  Alternative Title : Astrophys. J.
Source Genre: Journal
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Pages: - Volume / Issue: 639 (1 Part 2) Sequence Number: - Start / End Page: L1 - L4 Identifier: ISSN: 0067-0049