about
18 years of science with the Hubble Space Telescope.The formation and assembly of a typical star-forming galaxy at redshift z approximately 3.Galaxy Zoo: CANDELS barred discs and bar fractionsThe James Webb Space TelescopeDeep submillimeter images of NGC 7331; dust at the periphery of spiral disksNewborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?Tidal dwarf galaxies in the nearby UniverseA coincidence of disturbed morphology and blue UV colour: minor-merger-driven star formation in early-type galaxies at z∼ 0.6The WiggleZ Dark Energy Survey: high-resolution kinematics of luminous star-forming galaxiesInvestigating emission-line galaxy surveys with the Sloan Digital Sky Survey infrastructureMegaMorph: classifying galaxy morphology using multi-wavelength Sérsic profile fitsAGN host galaxies at redshiftz ≈ 0.7: peculiar or not?Cosmic evolution of the galaxy's mass and luminosity functions by morphological type from multi-wavelength data in the CDF-SouthObservational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 GyrThe tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep FieldThe structures of distant galaxies - V. The evolution of galaxy structure in stellar mass at z<1The importance of minor-merger-driven star formation and black hole growth in disc galaxiesListening to galaxies tuning atz~ 2.5–3.0: The first strikes of the Hubble forkVariations in 24-μm morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: new insights into the Hubble sequenceThe VIMOS Public Extragalactic Redshift Survey (VIPERS)The end of the beginningsClumpy star-forming regions as the origin of the peculiar morphology of high-redshift galaxiesThe SAMI Galaxy Survey: asymmetry in gas kinematics and its links to stellar mass and star formationDYNAMO-HST survey: clumps in nearby massive turbulent discs and the effects of clump clustering on kiloparsec scale measurements of clumpsDYNAMO – I. A sample of Hα-luminous galaxies with resolved kinematicsHubble Space Telescope imaging of the CFRS and LDSS redshift surveys--IV. Influence of mergers in the evolution of faint field galaxies from z 1
P2860
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P2860
description
im April 1996 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у квітні 1996
@uk
name
Galaxy morphology to I=25 mag in the Hubble Deep Field
@en
Galaxy morphology to I=25 mag in the Hubble Deep Field
@nl
type
label
Galaxy morphology to I=25 mag in the Hubble Deep Field
@en
Galaxy morphology to I=25 mag in the Hubble Deep Field
@nl
prefLabel
Galaxy morphology to I=25 mag in the Hubble Deep Field
@en
Galaxy morphology to I=25 mag in the Hubble Deep Field
@nl
P2093
P356
P1476
Galaxy morphology to I=25 mag in the Hubble Deep Field
@en
P2093
B. X. Santiago
K. Glazebrook
N. R. Tanvir
R. G. Abraham
R. S. Ellis
S. v. d. Bergh
P356
10.1093/MNRAS/279.3.L47
P407
P577
1996-04-01T00:00:00Z
P818
astro-ph/9602044
P819
1996MNRAS.279L..47A