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  Evolution of the most massive galaxies to z= 0.6 – I. A new method for physical parameter estimation

Chen, Y.-M., Kauffmann, G., Tremonti, C. A., White, S., Heckman, T. M., Kovac, K., et al. (2012). Evolution of the most massive galaxies to z= 0.6 – I. A new method for physical parameter estimation. Monthly Notices of the Royal Astronomical Society, 421(1), 314-332. doi:10.1111/j.1365-2966.2011.20306.x.

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 Creators:
Chen, Yan-Mei, Author
Kauffmann, Guinevere1, Author              
Tremonti, Christy A., Author
White, Simon1, Author              
Heckman, Timothy M., Author
Kovac, Katarina1, Author              
Bundy, Kevin, Author
Chisholm, John, Author
Maraston, Claudia, Author
Schneider, Donald P., Author
Bolton, Adam S., Author
Weaver, Benjamin A., Author
Brinkmann, Jon, Author
Affiliations:
1Cosmology, MPI for Astrophysics, Max Planck Society, ou_159876              

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Language(s): eng - English
 Dates: 2012-03
 Publication Status: Published in print
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 Rev. Type: Peer
 Identifiers: DOI: 10.1111/j.1365-2966.2011.20306.x
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. R. Astr. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 421 (1) Sequence Number: - Start / End Page: 314 - 332 Identifier: ISSN: 0035-8711