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Luminosity function constraints on the evolution of massive red galaxies since z∼ 0.9

Cool, Richard J.; Eisenstein, Daniel J.; Fan, Xiaohui; Fukugita, Masataka; Jiang, Linhua; Maraston, Claudia; Meiksin, Avery; Schneider, Donald P. and Wake, David A. (2008). Luminosity function constraints on the evolution of massive red galaxies since z∼ 0.9. Astrophysical Journal, 682(2) pp. 919–936.

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DOI (Digital Object Identifier) Link: https://doi.org/10.1086/589642
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Abstract

We measure the evolution of the luminous red galaxy (LRG) luminosity function in the redshift range 0.1 < z < 0.9 using samples of galaxies from the Sloan Digital Sky Survey as well as new spectroscopy of high-redshift massive red galaxies. Our high-redshift sample of galaxies is largest spectroscopic sample of massive red galaxies at z ~ 0.9 collected to date and covers 7 deg2, minimizing the impact of large-scale structure on our results. We find that the LRG population has evolved little beyond the passive fading of its stellar populations since z ~ 0.9. Based on our luminosity function measurements and assuming a nonevolving Salpeter stellar initial mass function, we find that the most massive (L > 3L*) red galaxies have grown by less than 50% (at 99% confidence), since z = 0.9, in stark contrast to the factor of 2-4 growth observed in the L* red galaxy population over the same epoch. We also investigate the evolution of the average LRG spectrum since z ~ 0.9 and find the high-redshift composite to be well described as a passively evolving example of the composite galaxy observed at low redshift. From spectral fits to the composite spectra, we find at most 5% of the stellar mass in massive red galaxies may have formed within 1 Gyr of z = 0.9. While L* red galaxies are clearly assembled at z < 1, 3L* galaxies appear to be largely in place and evolve little beyond the passive evolution of their stellar populations over the last half of cosmic history.

Item Type: Journal Item
Copyright Holders: 2008. The American Astronomical Society.
ISSN: 1538-4357
Keywords: elliptical galaxies; lenticular galaxies; cD; evolution; fundamental parameters; photometry
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 38511
Depositing User: Miranda Callaway
Date Deposited: 20 Sep 2013 14:38
Last Modified: 07 Dec 2018 16:35
URI: http://oro.open.ac.uk/id/eprint/38511
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