Results 181 to 190 of about 16,096,383 (218)

Spectroscopic confirmation of two luminous galaxies at a redshift of 14. [PDF]

open access: yesNature
Carniani S   +44 more
europepmc   +1 more source

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]

open access: yesOpen Res Eur
Di Mascolo L   +26 more
europepmc   +1 more source

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

open access: yes
Fujimoto S   +45 more
europepmc   +1 more source

Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing. [PDF]

open access: yesSpace Sci Rev
Birrer S   +8 more
europepmc   +1 more source

High redshift X-ray galaxy clusters [PDF]

open access: yesAstronomy and Astrophysics, 2007
The current generation of X-ray observatories like Chandra allows studies with very fine spatial details. It is now possible to resolve X-ray point sources projected into the cluster diffuse emission and exclude them from the analysis to estimate the ``correct'' X-ray observables. In order to verify the incidence of point sources on the cluster thermal
Isabella M. Gioia, R Fanti
exaly   +6 more sources

The mass–concentration relation in massive galaxy clusters at redshift ∼1

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
Mass and concentration of clusters of galaxies are related and evolving with redshift. We study the properties of a sample of 31 massive galaxy clusters at high redshift, 0.8 < ∼ z < ∼ 1.5, using weak and strong lensing observations.
Giovanni Covone, Mauro Sereno
exaly   +2 more sources

What are protoclusters? – Defining high-redshift galaxy clusters and protoclusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
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 $z=2$ ($\sim30\, \rm{arcmin}$).
Nina Hatch, Elizabeth Cooke
exaly   +5 more sources

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