Non-Separable Halo Bias from High-Redshift Galaxy Clustering
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
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BeppoSAX observations of two high redshift clusters of galaxies: RXJ0152.7-1357 and MS2053.7-0449 [PDF]
R. Della Ceca +5 more
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Detecting Clusters of Galaxies at High Redshift with the Spitzer Space Telescope [PDF]
Gillian Wilson +3 more
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Clustering analysis of medium-band selected high-redshift galaxies
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
A rising tide: intrinsic alignments since the turn of the millennium. [PDF]
Chisari NE.
europepmc +1 more source
THEXMMCLUSTER SURVEY: THE BUILD-UP OF STELLAR MASS IN BRIGHTEST CLUSTER GALAXIES AT HIGH REDSHIFT [PDF]
J. P. Stott +16 more
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The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]
Taylor ED +9 more
europepmc +1 more source
Photometric Redshifts in lensing clusters: Identification and\n Calibration of faint high-z galaxies [PDF]
R. Pelló +3 more
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Comparing the motion of dark matter and standard model particles on cosmological scales. [PDF]
Grimm N, Bonvin C, Tutusaus I.
europepmc +1 more source
Submillimetre source counts in the fields of high-redshift galaxy clusters [PDF]
Allison Noble +13 more
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