The structures of distant galaxies – I. Galaxy structures and the merger rate to z ∼ 3 in the Hubble Ultra-Deep Field
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The effects of a hot gaseous halo in galaxy major mergersThe merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS surveyThe properties of the star-forming interstellar medium atz = 0.84-2.23 from HiZELS: mapping the internal dynamics and metallicity gradients in high-redshift disc galaxiesA chronicle of galaxy mass assembly in the EAGLE simulationTidal dwarf galaxies in the nearby UniverseGalaxy Zoo: multimergers and the Millennium SimulationGalaxy Zoo: an independent look at the evolution of the bar fraction over the last eight billion years from HST-COSMOS★Morphological classification of local luminous infrared galaxiesMASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assemby Survey with SINFONI in VVDSExploring the progenitors of brightest cluster galaxies atz ∼ 2A new automatic method to identify galaxy mergers - I. Description and application to the Space Telescope A901/902 Galaxy Evolution Survey★ASTErIsM: application of topometric clustering algorithms in automatic galaxy detection and classificationThe 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 < 3.5New image statistics for detecting disturbed galaxy morphologies at high redshiftThe redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDSThe tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep FieldGalaxy properties in different environments up to z∼ 3 in the GOODS NICMOS SurveyHow do Galaxies get their Baryons?Observations and modeling of a clumpy galaxy at z = 1.6. Spectroscopic clues to the origin and evolution of chain galaxiesThe limited role of galaxy mergers in driving stellar mass growth over cosmic timeGas accretion as a dominant formation mode in massive galaxies from the GOODS NICMOS SurveyWide and deep near-UV (360 nm) galaxy counts and the extragalactic background light with the Large Binocular CameraListening to galaxies tuning atz~ 2.5–3.0: The first strikes of the Hubble forkThe ALHAMBRA survey: accurate merger fractions derived by PDF analysis of photometrically close pairsThe impact from survey depth and resolution on the morphological classification of galaxiesThe SAMI Galaxy Survey: asymmetry in gas kinematics and its links to stellar mass and star formationThe Dawes Review 1: Kinematic Studies of Star-Forming Galaxies Across Cosmic Time
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The structures of distant galaxies – I. Galaxy structures and the merger rate to z ∼ 3 in the Hubble Ultra-Deep Field
description
article
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im Mai 2008 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в травні 2008
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The structures of distant gala ...... in the Hubble Ultra-Deep Field
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The structures of distant gala ...... in the Hubble Ultra-Deep Field
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type
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The structures of distant gala ...... in the Hubble Ultra-Deep Field
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The structures of distant gala ...... in the Hubble Ultra-Deep Field
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The structures of distant gala ...... in the Hubble Ultra-Deep Field
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The structures of distant gala ...... in the Hubble Ultra-Deep Field
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P2860
P1476
The structures of distant gala ...... in the Hubble Ultra-Deep Field
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P2093
Robert Myers
Sheena Rajgor
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P304
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10.1111/J.1365-2966.2008.13069.X
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P577
2008-05-01T00:00:00Z
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P819
2008MNRAS.386..909C