output
20022026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2018 · astro-ph.COShow all

12 papers · 2 filters

astro-ph.CO2018★ 28 cited

Large-Scale Velocity Dispersion and the Cosmic Web

Michael Buehlmann, Oliver Hahn

Gravitational collapse in cosmological context produces an intricate cosmic web of voids, walls, filaments and nodes. The anisotropic nature of collisionless collapse leads to the…

astro-ph.CO2018★ 28 cited

Semiclassical path to cosmic large-scale structure

Cora Uhlemann, Cornelius Rampf, Mateja Gosenca +1

We chart a path toward solving for the nonlinear gravitational dynamics of cold dark matter by relying on a semiclassical description using the propagator. The evolution of the pro…

astro-ph.CO2018★ 131 cited

The XXL Survey XX: The 365 cluster catalogue

C. Adami, P. Giles, E. Koulouridis +54

In the currently debated context of using clusters of galaxies as cosmological probes, the need for well-defined cluster samples is critical. The XXL Survey has been specifically d…

astro-ph.CO2018★ 10 cited

Gaia GraL: Gaia DR2 Gravitational Lens Systems. IV. Keck/LRIS spectroscopic confirmation of GRAL113100-441959 and model prediction of time-delays

Olivier Wertz, Daniel Stern, Alberto Krone-Martins +14

We report the spectroscopic confirmation and modeling of the quadruply imaged quasar GRAL113100-441959, the first gravitational lens (GL) to be discovered mainly from astrometric c…

astro-ph.CO2018★ 79 cited

The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts

F. Pacaud, M. Pierre, J. -B. Melin +25

Context. We present an estimation of cosmological parameters with clusters of galaxies. Aims. We constrain the , , and parameters from a stand-alone sample of X-ray c…

astro-ph.CO2018★ 6 cited

A Relativistic Interpretation of Bias in Newtonian Simulations

Christian Fidler, Nils Sujata, Cornelius Rampf

Observables of cosmic structures are usually not the underlying matter field but biased tracers of matter, such as galaxies or halos. We show how the bias found in Newtonian N-body…