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Measuring the average evolution of luminous galaxies at z < 3: the rest-frame optical luminosity density, spectral energy distribution, and stellar mass density

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Förster Schreiber,  Natascha M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Rudnick, G., Labbé, I., Förster Schreiber, N. M., Wuyts, S., Franx, M., Finlator, K., et al. (2006). Measuring the average evolution of luminous galaxies at z < 3: the rest-frame optical luminosity density, spectral energy distribution, and stellar mass density. Astrophysical Journal, 650(2 Part 1), 624-643. doi:10.1086/507123.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-D258-E
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