output
19932026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2019 · astro-ph.COShow all

40 papers · 2 filters

astro-ph.CO2019★ 34 cited

Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys

Mario Ballardini, Riccardo Murgia, Marco Baldi +2

Galaxy surveys are an important probe for superimposed oscillations on the primordial power spectrum of curvature perturbations, which are predicted in several theoretical models o…

astro-ph.CO2019★ 12 cited

Calibration of systematics in constraining modified gravity models with galaxy cluster mass profiles

L. Pizzuti, B. Sartoris, S. Borgani +1

Joint lensing and dynamical mass profile determinations of galaxy clusters are an excellent tool to constrain modification of gravity at cosmological scales. However, search for ti…

astro-ph.CO2019★ 32 cited

Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments

A. C. Deshpande, T. D. Kitching, V. F. Cardone +69

Stage IV weak lensing experiments will offer more than an order of magnitude leap in precision. We must therefore ensure that our analyses remain accurate in this new era. Accordin…

astro-ph.CO2019★ 64 cited

CODEX clusters. The Survey, the Catalog, and Cosmology of the X-ray Luminosity Function

A. Finoguenov, E. Rykoff, N. Clerc +17

Large area catalogs of galaxy clusters constructed from ROSAT All Sky Survey provide the base for our knowledge on the population of clusters thanks to the long-term multiwavelengt…

astro-ph.CO2019★ 14 cited

RELICS: A Very Large () Cluster Lens -- RXC J0032.1+1808

Ana Acebron, Adi Zitrin, Dan Coe +38

Extensive surveys with the \textit{Hubble Space Telescope} (HST) over the past decade, targeting some of the most massive clusters in the sky, have uncovered dozens of galaxy-clust…

astro-ph.CO2019★ 12 cited

The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation

R. Thomas, L. Pentericci, O. Le Fèvre +22

Aims. Our aim is to estimate the intergalactic medium transmission towards UV-selected star-forming galaxies at redshift 4 and above and study the effect of the dust attenuation on…