activity
20142026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 3.1k across the 264 of their papers we have counts for

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Showing 2020Show all

10 papers · 1 filter

astro-ph.CO2020★ 166 cited

Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations

Euclid Collaboration, M. Knabenhans, J. Stadel +131

We present a new, updated version of the EuclidEmulator (called EuclidEmulator2), a fast and accurate predictor for the nonlinear correction of the matter power spectrum. Percent-l…

astro-ph.GA2020★ 8 cited

On the reliability of photometric and spectroscopic tracers of halo relaxation

Mohammad H. Zhoolideh Haghighi, Mojtaba Raouf, Habib. G. Khosroshahi +2

We characterize the relaxation state of galaxy systems by providing an assessment of the reliability of the photometric and spectroscopic probe via the semi-analytic galaxy evoluti…

astro-ph.GA2020★ 114 cited

Euclid preparation: X. The Euclid photometric-redshift challenge

Euclid Collaboration, G. Desprez, S. Paltani +170

Forthcoming large photometric surveys for cosmology require precise and accurate photometric redshift (photo-z) measurements for the success of their main science objectives. Howev…

astro-ph.GA2020★ 22 cited

FR-type radio sources at 3 GHz VLA-COSMOS: Relation to physical properties and large-scale environment

E. Vardoulaki, E. F. Jiménez Andrade, I. Delvecchio +16

() We probe the physical properties and large-scale environment of radio AGN in the faintest FR population to-date, and link them to their radio structure. We use the VLA…

astro-ph.CO2020★ 55 cited

Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA

Johan Comparat, Dominique Eckert, Alexis Finoguenov +25

The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) mission will measure the position and properties of about 100,000 clusters of galaxies and 3 million active g…

astro-ph.GA2020★ 21 cited

The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups

T. Pasini, M. Brūggen, F. de Gasperin +10

Our understanding of how AGN feedback operates in galaxy clusters has improved in recent years owing to large efforts in multi-wavelength observations and hydrodynamical simulation…