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• W3105372211 endingPage "92" @default.
• W3105372211 startingPage "92" @default.
• W3105372211 abstract "[Abridged] Using public data from the NMBS and CANDELS surveys, we study the population of massive galaxies at z>3 to identify the potential progenitors of z~2 compact, massive, quiescent (CMQ) galaxies, furthering our understanding of the evolution of massive galaxies. Our work is enabled by high-resolution CANDELS images and accurate photometric redshifts, stellar masses and star formation rates (SFRs) from 37-band NMBS photometry. The total number of z>3 massive galaxies is consistent with the number of massive quiescent (MQ) galaxies at z~2, implying that the SFRs for all of these galaxies must be much lower by z~2. We discover 4 CMQ galaxies at z>3, pushing back the time for which such galaxies have been observed. However, the volume density for these galaxies is significantly less than that of galaxies at z<2 with similar masses, SFRs, and sizes, implying that additional CMQ galaxies must be created in the ~1 Gyr between z=3 and z=2. We find 5 star-forming galaxies at z~3 that are compact (Re<1.4 kpc) and have stellar mass M*>10^(10.6)Msun, likely to become members of the CMQ galaxy population at z~2. We evolve the stellar masses and SFRs of each individual z>3 galaxy adopting 5 different star formation histories (SFHs) and studying the resulting population of massive galaxies at z=2.3. We find that declining or truncated SFHs are necessary to match the observed number density of MQ galaxies at z~2, whereas a constant SFH results in a number density significantly smaller than observed. All of our assumed SFHs imply number densities of CMQ galaxies at z~2 that are consistent with the observed number density. Better agreement with the observed number density of CMQ galaxies at z~2 is obtained if merging is included in the analysis and better still if star formation quenching is assumed to shortly follow the merging event, as implied by recent models of formation of MQ galaxies." @default.
• W3105372211 created "2020-11-23" @default.
• W3105372211 creator A5016434271 @default.
• W3105372211 creator A5021395641 @default.
• W3105372211 creator A5043012847 @default.
• W3105372211 creator A5072732930 @default.
• W3105372211 creator A5080276340 @default.
• W3105372211 date "2013-04-17" @default.
• W3105372211 modified "2023-09-23" @default.
• W3105372211 title "WHAT ARE THE PROGENITORS OF COMPACT, MASSIVE, QUIESCENT GALAXIES AT<i>z</i>= 2.3? THE POPULATION OF MASSIVE GALAXIES AT<i>z</i>> 3 FROM NMBS AND CANDELS" @default.
• W3105372211 cites W1969214334 @default.
• W3105372211 cites W1970196846 @default.
• W3105372211 cites W1972726718 @default.
• W3105372211 cites W1979789803 @default.
• W3105372211 cites W1981452559 @default.
• W3105372211 cites W1994671833 @default.
• W3105372211 cites W1996926090 @default.
• W3105372211 cites W2004084407 @default.
• W3105372211 cites W2015295900 @default.
• W3105372211 cites W2025020969 @default.
• W3105372211 cites W2033803356 @default.
• W3105372211 cites W2051907193 @default.
• W3105372211 cites W2054131667 @default.
• W3105372211 cites W2064449842 @default.
• W3105372211 cites W2066613100 @default.
• W3105372211 cites W2067195208 @default.
• W3105372211 cites W2069396164 @default.
• W3105372211 cites W2079227246 @default.
• W3105372211 cites W2089191176 @default.
• W3105372211 cites W2093468672 @default.
• W3105372211 cites W2110974947 @default.
• W3105372211 cites W2112370854 @default.
• W3105372211 cites W2112633422 @default.
• W3105372211 cites W2114350853 @default.
• W3105372211 cites W2115927937 @default.
• W3105372211 cites W2117885077 @default.
• W3105372211 cites W2129760210 @default.
• W3105372211 cites W2135052708 @default.
• W3105372211 cites W2139105939 @default.
• W3105372211 cites W2142238829 @default.
• W3105372211 cites W2147803603 @default.
• W3105372211 cites W2149653371 @default.
• W3105372211 cites W2149739542 @default.
• W3105372211 cites W2150772486 @default.
• W3105372211 cites W2153037851 @default.
• W3105372211 cites W2153886904 @default.
• W3105372211 cites W2155416414 @default.
• W3105372211 cites W2155704245 @default.
• W3105372211 cites W2155705849 @default.
• W3105372211 cites W2158454843 @default.
• W3105372211 cites W2158528198 @default.
• W3105372211 cites W2162399571 @default.
• W3105372211 cites W2165084703 @default.
• W3105372211 cites W2166618419 @default.
• W3105372211 cites W2167098341 @default.
• W3105372211 cites W2233307855 @default.
• W3105372211 cites W3098220822 @default.
• W3105372211 cites W3098648953 @default.
• W3105372211 cites W3098964905 @default.
• W3105372211 cites W3099020958 @default.
• W3105372211 cites W3099172813 @default.
• W3105372211 cites W3099396163 @default.
• W3105372211 cites W3101562594 @default.
• W3105372211 cites W3102970349 @default.
• W3105372211 cites W3103332895 @default.
• W3105372211 cites W3103596053 @default.
• W3105372211 cites W3103650992 @default.
• W3105372211 cites W3104846156 @default.
• W3105372211 cites W3105413605 @default.
• W3105372211 cites W3105517603 @default.
• W3105372211 cites W3105731735 @default.
• W3105372211 cites W3105889752 @default.
• W3105372211 cites W3106428543 @default.
• W3105372211 cites W3106464621 @default.
• W3105372211 cites W3115804805 @default.
• W3105372211 cites W3121715540 @default.
• W3105372211 cites W3121928262 @default.
• W3105372211 cites W3122319269 @default.
• W3105372211 cites W3123341302 @default.
• W3105372211 cites W3124028209 @default.
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• W3105372211 cites W3125341864 @default.
• W3105372211 cites W4298348205 @default.
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• W3105372211 doi "https://doi.org/10.1088/0004-637x/768/1/92" @default.
• W3105372211 hasPublicationYear "2013" @default.
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