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

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http://pubman.mpdl.mpg.de/cone/persons/resource/persons4706

Kauffmann,  Guinevere
Cosmology, MPI for Astrophysics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4755

White,  Simon
Cosmology, MPI for Astrophysics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons45847

Kovac,  Katarina
Cosmology, MPI for Astrophysics, Max Planck Society;

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Citation

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.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-C44C-2
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