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galaxies: high-redshif

Herschel ATLAS: properties of dusty massive galaxies at low and high redshifts

Herschel ATLAS: properties of dusty massive galaxies at low and high redshifts

... of high-redshift submillimetre galaxies (SMGs) with robust optical counterparts and spectroscopic redshifts in the ...the galaxies in our sample have well-sampled cov- erage of the peak of the dust ...

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Ultra red Galaxies Signpost Candidate Protoclusters at High Redshift

Ultra red Galaxies Signpost Candidate Protoclusters at High Redshift

... ultra-red galaxies do indeed trace the precursors of the most massive ETGs in the centers of present-day galaxy clusters, we would expect to witness unvirialized systems characterized by overdensities of ( ...

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Reionization and high redshift galaxies: the view from quasar absorption lines

Reionization and high redshift galaxies: the view from quasar absorption lines

... of high-redshift galaxy candidates – some of which are spectroscopically confirmed – using the Lyman-break technique (see also ...Lyman-break galaxies (LBGs) at rest-frame wavelength of 1500 ˚ A out to z ∼ 8 ...

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High Redshift Galaxies As Probes Of The Epoch Of Reionization

High Redshift Galaxies As Probes Of The Epoch Of Reionization

... redshift galaxies, the [CII] line is a strong cooling line with a luminosity that is ...selected galaxies and quasar host galaxies at z & 6, although there are also a handful of upper limits ...

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The interstellar medium in high redshift submillimeter galaxies as probed by infrared spectroscopy

The interstellar medium in high redshift submillimeter galaxies as probed by infrared spectroscopy

... of galaxies and consequently manifest in the relative strengths of fi ne structure emission ...for high-redshift galaxies prior to ...brightest galaxies — primarily gravitationally lensed ...in ...

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The Interstellar Medium in High redshift Submillimeter Galaxies as Probed by Infrared Spectroscopy*

The Interstellar Medium in High redshift Submillimeter Galaxies as Probed by Infrared Spectroscopy*

... targeting high-redshift star-forming galaxies ...targeted galaxies, in terms of the IR-luminosity and redshift distributions, and with IR emission being dominated by ...

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Detailed Properties of High Redshift Galaxies

Detailed Properties of High Redshift Galaxies

... forming galaxies at z ≃ 2 − 3 based on a modest ...massive galaxies at similar redshifts ...forming galaxies at this epoch are undergoing mergers while the remaining ∼ 2/3 are isolated with ...

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Lyman Continuum and Lyman α Emission from Galaxies at High Redshift

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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The dust budget crisis in high redshift submillimetre galaxies

The dust budget crisis in high redshift submillimetre galaxies

... reality, galaxies are unlikely to be closed systems ...for galaxies at a fixed gas-phase oxygen abundance (Gallazzi et ...at high redshift provide further indirect evidence that inflows are required, ...

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Ultra red Galaxies Signpost Candidate Protoclusters at High Redshift

Ultra red Galaxies Signpost Candidate Protoclusters at High Redshift

... – The Fourier spectrum of the timestreams were high-pass filtered below 0.5 Hz using a noise- whitening algorithm to remove the 1/f noise. At this stage, the mean noise-weighted point-source sensitivity of all ...

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The Kiloparsec Scale Structure and Kinematics of High Redshift Star Forming Galaxies

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 thought to ...

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De Lucia, Gabriella
  

(2004):


	Evolution of Galaxies in Clusters.


Dissertation, LMU München: Fakultät für Physik

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 high ...

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The Intergalactic and Circumgalactic Medium Surrounding Star-Forming Galaxies at Redshifts 2

The Intergalactic and Circumgalactic Medium Surrounding Star-Forming Galaxies at Redshifts 2<z<3

... study high-z galaxies and their intergalactic environs have been made by Adelberger et ...forming galaxies at high redshift, and, perhaps more tantalizing, evidence for interactions between ...

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Galaxies in X ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red Sequence Galaxy Luminosity Function

Galaxies in X ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red Sequence Galaxy Luminosity Function

... At intermediate to high redshift, measurements of RSLF are still scarce. Sample sizes used in previous works are much smaller than those in SDSS-based studies. Any mass dependent effect of α would make it ...

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Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z

Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z <0 5

... of galaxies at high redshift. Observationally, galax- ies at high redshift observed in the HDF or UDF with the Hubble Space Telescope (HST) show clumpy structures with high star formation ...

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Galaxy And Mass Assembly (GAMA): the wavelength dependent sizes and profiles of galaxies revealed by MegaMorph

Galaxy And Mass Assembly (GAMA): the wavelength dependent sizes and profiles of galaxies revealed by MegaMorph

... mass galaxies (both star forming and passive) contain younger and lower metallicity stellar populations, and are there- fore bluer in colour ...merging galaxies originate increases with ...to ...

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Multi Wavelength Properties of Submillimeter Selected Galaxies

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 ...templates. ...

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A mature galaxy cluster at z= 1 58 around the radio galaxy 7C 1753+6311

A mature galaxy cluster at z= 1 58 around the radio galaxy 7C 1753+6311

... of galaxies in the densest environments, clusters, it is important to study their progenitors: high-redshift protocluster ...The high-redshift progenitors of the majority of local M ∼ 10 14 M e ...

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Chemical evolution of star-forming galaxies in the overdense environment

Chemical evolution of star-forming galaxies in the overdense environment

... cluster galaxies is intimately linked with the local ICM properties of the ...in galaxies as a function of the ICM density (or cluster-centric distance), there- fore provide new insights into the interplay ...

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Near ultraviolet signatures of environment driven galaxy quenching in Sloan Digital Sky Survey groups

Near ultraviolet signatures of environment driven galaxy quenching in Sloan Digital Sky Survey groups

... 2014). Galaxies in the green valley have shown intermediate specific star formation rates (log(sSFR)∼ −11), red optical colours, and intermediate masses (M ∼ 10 ...

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