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• W3100588152 abstract "We present a comparison between the observed color distribution, number and mass density of massive galaxies at 1.5 4x10^10 Msun) galaxies extracted from the FIRES, GOODS-South, and MUSYC surveys, together spanning an area of 496 arcmin^2, with synthetic photometry from hydrodynamical merger simulations. As in the Hopkins et al. (2006b) model, we use the observed quasar luminosity function to estimate the merger rate. We find that the synthetic U-V and V-J colors of galaxies that had a quasar phase in their past match the colors of observed galaxies that are best characterized by a quiescent stellar population. At z ~ 2.6, the observed number and mass density of quiescent red galaxies with M > 4x10^10 Msun is consistent with the model in which every quiescent massive galaxy underwent a quasar phase in the past. At z ~ 1.9, 2.8 times less quiescent galaxies are observed than predicted by the model as descendants of higher redshift quasars. The merger model also predicts a large number of galaxies undergoing merger-driven star formation. We find that the predicted number and mass density accounts for 30-50% of the observed massive star-forming galaxies. However, their colors do not match those of observed star-forming galaxies. In particular, the colors of dusty red galaxies are not reproduced by the simulations. Several possible origins of this discrepancy are discussed. The observational constraints on the validity of the model are currently limited by cosmic variance and uncertainties in stellar population synthesis and radiative transfer." @default.
• W3100588152 created "2020-11-23" @default.
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• W3100588152 date "2009-07-06" @default.
• W3100588152 modified "2023-09-27" @default.
• W3100588152 title "COLOR DISTRIBUTIONS, NUMBER, AND MASS DENSITIES OF MASSIVE GALAXIES AT 1.5 <z< 3: COMPARING OBSERVATIONS WITH MERGER SIMULATIONS" @default.
• W3100588152 cites W1492683732 @default.
• W3100588152 cites W1964084977 @default.
• W3100588152 cites W1964844412 @default.
• W3100588152 cites W1965134192 @default.
• W3100588152 cites W1970333333 @default.
• W3100588152 cites W1970660289 @default.
• W3100588152 cites W1972308849 @default.
• W3100588152 cites W1973939397 @default.
• W3100588152 cites W1980924370 @default.
• W3100588152 cites W1986486448 @default.
• W3100588152 cites W1990479252 @default.
• W3100588152 cites W1992635601 @default.
• W3100588152 cites W1992861681 @default.
• W3100588152 cites W1994662943 @default.
• W3100588152 cites W1994703407 @default.
• W3100588152 cites W1999296210 @default.
• W3100588152 cites W1999624500 @default.
• W3100588152 cites W2001085255 @default.
• W3100588152 cites W2002044265 @default.
• W3100588152 cites W2004084407 @default.
• W3100588152 cites W2006316173 @default.
• W3100588152 cites W2012886609 @default.
• W3100588152 cites W2012983802 @default.
• W3100588152 cites W2015295900 @default.
• W3100588152 cites W2015529116 @default.
• W3100588152 cites W2020380072 @default.
• W3100588152 cites W2020863669 @default.
• W3100588152 cites W2025458316 @default.
• W3100588152 cites W2025629511 @default.
• W3100588152 cites W2029965202 @default.
• W3100588152 cites W2032317739 @default.
• W3100588152 cites W2036319176 @default.
• W3100588152 cites W2037816996 @default.
• W3100588152 cites W2040759695 @default.
• W3100588152 cites W2043038124 @default.
• W3100588152 cites W2045895958 @default.
• W3100588152 cites W2064899774 @default.
• W3100588152 cites W2066886457 @default.
• W3100588152 cites W2070276447 @default.
• W3100588152 cites W2070431442 @default.
• W3100588152 cites W2072801955 @default.
• W3100588152 cites W2080977367 @default.
• W3100588152 cites W2081243021 @default.
• W3100588152 cites W2081425105 @default.
• W3100588152 cites W2089167229 @default.
• W3100588152 cites W2090459210 @default.
• W3100588152 cites W2091867375 @default.
• W3100588152 cites W2092504858 @default.
• W3100588152 cites W2093468672 @default.
• W3100588152 cites W2098564368 @default.
• W3100588152 cites W2098600168 @default.
• W3100588152 cites W2100514692 @default.
• W3100588152 cites W2109146631 @default.
• W3100588152 cites W2109329782 @default.
• W3100588152 cites W2112341914 @default.
• W3100588152 cites W2120523711 @default.
• W3100588152 cites W2128904482 @default.
• W3100588152 cites W2129760210 @default.
• W3100588152 cites W2135052708 @default.
• W3100588152 cites W2135296228 @default.
• W3100588152 cites W2135894620 @default.
• W3100588152 cites W2137987137 @default.
• W3100588152 cites W2143283226 @default.
• W3100588152 cites W2144320326 @default.
• W3100588152 cites W2145024951 @default.
• W3100588152 cites W2150995848 @default.
• W3100588152 cites W2151062050 @default.
• W3100588152 cites W2154856197 @default.
• W3100588152 cites W2154955582 @default.
• W3100588152 cites W2160741239 @default.
• W3100588152 cites W2162125418 @default.
• W3100588152 cites W2162516451 @default.
• W3100588152 cites W2167262338 @default.
• W3100588152 cites W2168414272 @default.
• W3100588152 cites W2952200430 @default.
• W3100588152 cites W3098975407 @default.
• W3100588152 cites W3099136671 @default.
• W3100588152 cites W3099172813 @default.
• W3100588152 cites W3099267591 @default.
• W3100588152 cites W3099510124 @default.
• W3100588152 cites W3100679294 @default.

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