Results 151 to 160 of about 49,283 (254)

Non-Separable Halo Bias from High-Redshift Galaxy Clustering

open access: yes
The halo model provides a powerful framework for interpreting galaxy clustering by linking the spatial distribution of dark matter haloes to the underlying matter distribution. A key assumption within the linear bias approximation of the halo model is that the halo bias between two halo populations is a separable function of the mass of each population.
Mons, Emy   +3 more
openaire   +2 more sources

BeppoSAX observations of two high redshift clusters of galaxies: RXJ0152.7-1357 and MS2053.7-0449 [PDF]

open access: green, 1999
R. Della Ceca   +5 more
openalex   +1 more source

Detecting Clusters of Galaxies at High Redshift with the Spitzer Space Telescope [PDF]

open access: green, 2005
Gillian Wilson   +3 more
openalex   +1 more source

Clustering analysis of medium-band selected high-redshift galaxies

open access: yes
Next-generation large-scale structure spectroscopic surveys will probe cosmology at high redshifts $(2.3 < z < 3.5)$, relying on abundant galaxy tracers such as Ly$α$ emitters (LAEs) and Lyman break galaxies (LBGs). Medium-band photometry has emerged as a potential technique for efficiently selecting these high-redshift galaxies. In this work, we
Ebina, H.   +59 more
openaire   +2 more sources

THEXMMCLUSTER SURVEY: THE BUILD-UP OF STELLAR MASS IN BRIGHTEST CLUSTER GALAXIES AT HIGH REDSHIFT [PDF]

open access: bronze, 2010
J. P. Stott   +16 more
openalex   +1 more source

The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]

open access: yesNature
Taylor ED   +9 more
europepmc   +1 more source

Photometric Redshifts in lensing clusters: Identification and\n Calibration of faint high-z galaxies [PDF]

open access: green, 1999
R. Pelló   +3 more
openalex   +1 more source

Submillimetre source counts in the fields of high-redshift galaxy clusters [PDF]

open access: bronze, 2011
Allison Noble   +13 more
openalex   +1 more source

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