Results 11 to 20 of about 188 (137)
Studies of galaxy protoclusters yield insights into galaxy cluster formation complementary to those obtained via “archaeological” studies of present-day galaxy clusters.
Pablo Araya-Araya +8 more
doaj +3 more sources
Galaxy evolution in protoclusters [PDF]
14 pages, 9 figures, accepted for publication in ...
Stuart I. Muldrew +2 more
openaire +4 more sources
A Lyman-α protocluster at redshift 6.9 [PDF]
Comment: 9 pages, 5 figures, and 1 table.
Weida Hu +23 more
openaire +4 more sources
What are protoclusters? – Defining high-redshift galaxy clusters and protoclusters [PDF]
We explore the structures of protoclusters and their relationship with high redshift clusters using the Millennium Simulation combined with a semi-analytic model. We find that protoclusters are very extended, with 90 per cent of their mass spread across $\sim35\,h^{-1}{\rm Mpc}$ comoving at $z=2$ ($\sim30\, \rm{arcmin}$).
Muldrew, Stuart I. +2 more
openaire +5 more sources
Are Ly α emitters segregated in protoclusters regions? [PDF]
ABSTRACT The presence of neutral hydrogen in the interstellar medium (ISM) and intergalactic medium (IGM) induces radiative transfer (RT) effects on $\rm {Ly}\,\alpha$ photons that affect the observability of Lyman alpha emitters (LAEs). We use the galform semi-analytic model of galaxy formation and evolution to analyse how these effects
Tomás Hough +5 more
openaire +6 more sources
Characterising and identifying galaxy protoclusters [PDF]
19 pages, 16 figures, submitted to ...
Christopher C Lovell +2 more
openaire +2 more sources
A PROTOCLUSTER ATz= 2.45 [PDF]
submitted to ...
Diener, C. +8 more
openaire +7 more sources
Protoclusters associated withz> 2 radio galaxies [PDF]
[Abridged] We present the results of a large program conducted with the Very Large Telescope and Keck telescope to search for forming clusters of galaxies near powerful radio galaxies at 2.0 < z < 5.2. We obtained narrow- and broad-band images of nine radio galaxies and their surroundings.
Venemans, B. P. +10 more
openaire +2 more sources
The abundance of lensing protoclusters [PDF]
Weak gravitational lensing provides a potentially powerful method for the detection of clusters. In addition to cluster candidates, a large number of objects with possibly no optical or X-ray component have been detected in shear-selected samples.
D'Aloisio, Anson +2 more
openaire +2 more sources
LCDM predictions for galaxy protoclusters I: the relation between galaxies, protoclusters and quasars at z~6 [PDF]
Accepted by MNRAS (19 pages, 20 figures, 2 tables).
Overzier, R. +5 more
openaire +5 more sources

