Spectroscopic confirmation of two luminous galaxies at a redshift of 14. [PDF]
Carniani S +44 more
europepmc +1 more source
Imprints of massive black-hole binaries on neighbouring decihertz gravitational-wave sources. [PDF]
Stegmann J +4 more
europepmc +1 more source
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]
Di Mascolo L +26 more
europepmc +1 more source
Peaks in weak lensing mass maps for cluster astrophysics and cosmology. [PDF]
Oguri M, Miyazaki S.
europepmc +1 more source
Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
europepmc +1 more source
Counting Cosmic Cycles: Past Big Crunches, Future Recurrence Limits, and the Age of the Quantum Memory Matrix Universe. [PDF]
Neukart F, Marx E, Vinokur V.
europepmc +1 more source
Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing. [PDF]
Birrer S +8 more
europepmc +1 more source
High redshift X-ray galaxy clusters [PDF]
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
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]
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

