Strong size evolution of the most massive galaxies since z ∼ 2
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An evolutionary missing link? A modest-mass early-type galaxy hosting an oversized nuclear black holeIs there substructure around M87?Herschel reveals the obscured star formation in HiZELS H emitters at z = 1.47The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS surveyGalaxy size trends as a consequence of cosmologyAGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxiesMassive compact galaxies with high-velocity outflows: morphological analysis and constraints on AGN activityThe dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1The VIMOS VLT Deep SurveyExploring the progenitors of brightest cluster galaxies atz ∼ 2Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster SurveyA new automatic method to identify galaxy mergers - I. Description and application to the Space Telescope A901/902 Galaxy Evolution Survey★The fundamental plane of EDisCS galaxies. The effect of size evolutionThe Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5 < z < 3A consistent measure of the merger histories of massive galaxies using close-pair statistics – I. Major mergers at z < 3.5The effects of the cluster environment on the galaxy mass-size relation in MACS J1206.2-0847Galaxy And Mass Assembly (GAMA): $\mathcal {M_\star }\text{--}R_{\rm e}$ relations ofz= 0 bulges, discs and spheroidsGalaxy And Mass Assembly (GAMA): mass–size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphologyEarly-type galaxies have been the predominant morphological class for massive galaxies since only z ∼ 1Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model AnalysisStar formation and quenching among the most massive galaxies at z ∼ 1.7The host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACSThe decomposed bulge and disc size–mass relations of massive galaxies at 1 < z < 3 in CANDELSEvidence for two modes of black hole accretion in massive galaxies at z∼2The morphologies of massive galaxies at 1 <z< 3 in the CANDELS-UDS field: compact bulges, and the rise and fall of massive discsThe tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep FieldEvolution of massive galaxy structural properties and sizes via star formation in the GOODS NICMOS SurveyThe structures of distant galaxies – I. Galaxy structures and the merger rate to z ∼ 3 in the Hubble Ultra-Deep FieldALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75The sizes, masses and specific star formation rates of massive galaxies at 1.3 < z < 1.5: strong evidence in favour of evolution via minor mergersGas accretion as a dominant formation mode in massive galaxies from the GOODS NICMOS SurveySizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 atz= 1.39
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Strong size evolution of the most massive galaxies since z ∼ 2
description
im Oktober 2007 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в жовтні 2007
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name
Strong size evolution of the most massive galaxies since z ∼ 2
@en
Strong size evolution of the most massive galaxies since z ∼ 2
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type
label
Strong size evolution of the most massive galaxies since z ∼ 2
@en
Strong size evolution of the most massive galaxies since z ∼ 2
@nl
prefLabel
Strong size evolution of the most massive galaxies since z ∼ 2
@en
Strong size evolution of the most massive galaxies since z ∼ 2
@nl
P2093
P2860
P1476
Strong size evolution of the most massive galaxies since z ∼ 2
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P2093
Ignacio Trujillo
M. C. Cooper
P. Eisenhardt
Richard S. Ellis
P2860
P304
P356
10.1111/J.1365-2966.2007.12388.X
P407
P577
2007-10-30T00:00:00Z
P818
P819
2007MNRAS.382..109T