galaxies: evolution: galaxies: high-redshift
Kiloparsec-scale Dust Disks in High-redshift Luminous Submillimeter Galaxies
... resolve high-redshift galaxies except for in a handful of cases ( ...star-forming galaxies selected as likely progenitors of z ~ 2 compact quiescent galaxies — in the submillimeter ( ...
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Reionization and high redshift galaxies: the view from quasar absorption lines
... first galaxies reionized the intergalactic medium (IGM) promises to shed light on both the nature of the first objects and the cosmic history of ...between galaxies and the IGM near the reionization ...all ...
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Chan, Chi Chung (2016): Constraining the formation and evolution of cluster galaxies at z~1.5 using sizes and colour gradients. Dissertation, LMU München: Fakultät für Physik
... to redshift z ∼ 2 ...an evolution on the faint end of the luminosity function of the red sequence, which indicates a significant build up of the faint end of the red sequence towards lower redshift ...
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Multi Wavelength Properties of Submillimeter Selected Galaxies
... faint, high-redshift galaxies, whose submillimeter flux densities suggest large bolometric luminosities ( ∼ 10 13 L ) mostly emitted in IR wavebands, when SEDs of local ULIRGs were used as ...
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The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation
... around galaxies us- ing state-of-the-art cosmological hydrodynamical ...the Evolution and Assembly of Galaxies and their Environment (EAGLE) simulations (Schaye et ...relatively high ...
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The dust budget crisis in high redshift submillimetre galaxies
... chemical evolution, in reality, galaxies are unlikely to be closed systems ...for galaxies at a fixed gas-phase oxygen abundance (Gallazzi et ...at high redshift provide further ...
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The formation of bulges, discs and two-component galaxies in the CANDELS Survey at z < 3
... to high-redshift systems, where something more complicated, or a transition phase are potentially present between peculiar systems and the classic bulge + disc systems we see in today’s ...of ...
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One Plane for All: Massive Star-forming and Quiescent Galaxies Lie on the Same Mass Fundamental Plane at z ~ 0 and z ~ 0.7
... star-forming galaxies exist within the same 3D space, they still populate different regions of that ...of galaxies from one population may alter galaxy structures and dynamics and must do so within the ...
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A 6% measurement of the Hubble parameter at z~0 45 : direct evidence of the epoch of cosmic re acceleration
... which high-redshift ETGs are biased by sampling only the oldest and more massive progenitors of more local galaxies, therefore changing the slope of the age-redshift ...wide redshift ...
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Deep Infrared studies of massive high redshift galaxies
... and evolution of galaxies is a complex process, involving the growth of dark-matter structure from the gradual hierarchical merging of smaller fragments ...in galaxies, given the large parameter ...
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The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
... dSF galaxies increases with cosmic time, as expected from the observed metal enrichment with cosmic ...dSF galaxies tend to become the predominant type among the star-forming population at larger stellar ...
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Kakiichi, Koki (2016): The high redshift universe: galaxies and the intergalactic medium. Dissertation, LMU München: Fakultät für Physik
... universe, galaxies are only a minor ∼ 7% reservoir of the total baryons in the universe ([155, ...between galaxies in the form of the intergalactic medium (IGM). The evolution of the IGM is closely ...
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De Lucia, Gabriella (2004): Evolution of Galaxies in Clusters. Dissertation, LMU München: Fakultät für Physik
... at high redshift have been found by studying Lyman break galaxies ...relatively high (in the range ...these galaxies have been forming stars for more than 1 Gyr (Shapley et ...at ...
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Can planet formation resolve the dust budget crisis in high redshift galaxies?
... nearby galaxies (e.g. Andromeda, Mattsson et al. 2014) and the earliest galaxies (Wang, Hirashita & Hou 2017) suggest that grain growth (via accretion) would need to be responsible for ∼ 90 per cent of ...
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High Redshift Galaxies As Probes Of The Epoch Of Reionization
... and evolution of structure (Zaroubi ...satellite galaxies are actually observed (McQuinn ...satellite galaxies than might be expected for the same underlying dark matter halo ...
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Lyman Continuum and Lyman α Emission from Galaxies at High Redshift
... in galaxies, both locally and at high ...198 galaxies, members of a known proto-cluster in the field SSA22 (z ≈ ...Lyman-break galaxies (LBG) and 10 Lyman α ...“leaking” galaxies, we ...
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Detailed Properties of High Redshift Galaxies
... of galaxies from gravity alone, additional physical processes are required to explain the variety of observed baryonic properties of galaxies such as morphology, spectral energy distribution, and heavy ...
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The Kiloparsec Scale Structure and Kinematics of High Redshift Star Forming Galaxies
... earliest galaxies at redshift z ∼ 10 (see, ...early galaxies began to develop the orderly, regular morphological structures with which we are familiar in the local ...juvenile galaxies are ...
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An Empirically Calibrated Model for Interpreting the Evolution of Galaxies during the Reionization Era
... at high redshift and not probing an overdensity, then GGS should detect over 30 z ’ 8 Y 10 ...identifying galaxies at z ’ 7 Y 10 since they are able to reach sensitivity limits where objects are ...
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Ultra red Galaxies Signpost Candidate Protoclusters at High Redshift
... The evolution in overdensity increases ∼ 50 × from S ¢ = 7 16 mJy, although – the Poisson error from the blank- fi eld counts rises steeply at the higher fl ux densities, exacerbated by the large relative error in ...
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