The progenitors of present-day massive red galaxies up to z ≈ 0.7 - finding passive galaxies using SDSS-I/II and SDSS-III

Rita Tojeiro, Will Percival, D. Wake, Claudia Maraston, R. Skibba, I. Zehavi, Ashley Ross, J. Brinkmann, C. Conroy, H. Guo, Marc Manera, Karen Masters, Janine Pforr, Lado Samushia, D. Schneider, Daniel Thomas, B. Weaver, D. Bizyaev, H. Brewington, E. MalanushenkoV. Malanushenko, D. Oravetz, K. Pan, A. Shelden, A. Simmons, S. Snedden

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We present a comprehensive study of 250,000 galaxies targeted by the Baryon Oscillation Spectroscopic Survey (BOSS) up to z ~ 0.7 with the specific goal of identifying and characterising a population of galaxies that has evolved without significant merging. We compute a likelihood that each BOSS galaxy is a progenitor of the Luminous Red Galaxies (LRGs) sample, targeted by SDSS-I/II up z ~ 0.5, by using the fossil record of LRGs and their inferred star-formation histories, metallicity histories and dust content. We determine merger rates, luminosity growth rates and the evolution of the large-scale clustering between the two surveys, and we investigate the effect of using different stellar population synthesis models in our conclusions. We demonstrate that our sample is slowly evolving (of the order of 2 +/- 1.5% per Gyr by merging). Our conclusions refer to the bright and massive end of the galaxy population, with Mi0.55 < -22, and M* > 1E11.2 Msolar, corresponding roughly to 95% and 40% of the LRGs and BOSS galaxy populations, respectively. Our analysis further shows that any possible excess of flux in BOSS galaxies, when compared to LRGs, from potentially unresolved targets at z ~ 0.55 must be less than 1% in the r0.55-band (approximately equivalent to the g-band in the rest-frame of galaxies at z=0.55). When weighting the BOSS galaxies based on the predicted properties of the LRGs, and restricting the analysis to the reddest BOSS galaxies, we find an evolution of the large-scale clustering that is consistent with dynamical passive evolution, assuming a standard cosmology. We conclude that our likelihoods give a weighted sample that is as clean and as close to passive evolution (in dynamical terms, i.e. no or negligible merging) as possible, and that is optimal for cosmological studies.
Original languageEnglish
Pages (from-to)136-156
JournalMonthly Notices of the Royal Astronomical Society
Publication statusPublished - 2012


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