7 citations
- Centre National de la Recherche ScientifiqueFR32 papers
- Université de LilleFR31 papers
- Centre de Recherche en Informatique, Signal et Automatique de LilleFR28 papers
- Institut d'Astrophysique SpatialeFR22 papers
- Université Paris-SaclayFR22 papers
- Institute for Fundamental Physics of the UniverseIT21 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT21 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TriesteIT21 papers
- Ludwig-Maximilians-Universität MünchenDE21 papers
- Lyon 1 UniversitéFR21 papers
- National Institute for AstrophysicsIT21 papers
- Trieste Astronomical ObservatoryIT21 papers
17 papers · 1 filter
Gas motion in the intracluster medium of the Virgo cluster replica
Théo Lebeau, Stefano Ettori, Jenny G. Sorce +2
Within the deep gravitational potential of galaxy clusters lies the intracluster medium (ICM). At the first order, it is considered to be at hydrostatic equilibrium within the pote…
Euclid preparation. First investigation of the impact of cross-contamination on spectroscopic redshift measurements with pixel-level simulations
Euclid Collaboration, F. Passalacqua, S. Anselmi +299
We present a study on simulated data focused on understanding the performance of the spectroscopic redshift measurements with the Near-Infrared Spectrometer and Photometer (NISP) i…
Euclid. Populating a dark universe with galaxies using SciPIC
Euclid Collaboration, E. J. Gonzalez, J. Carretero +305
High-fidelity galaxy mocks are crucial for validating analysis pipelines and for cosmological inference. In this context, the Science Pipeline at PIC (SciPIC) is a pipeline specifi…
Euclid preparation. Decomposing components of the extragalactic background light using multi-band intensity mapping cross-correlations
Euclid Collaboration, Y. Cao, A. R. Cooray +269
The extragalactic background light (EBL) fluctuations in the optical/near-IR encode the cumulative integrated galaxy light (IGL), diffuse intra-halo light (IHL), and high- sourc…
Euclid preparation. Three-dimensional galaxy clustering in configuration space: Three-point correlation function estimation
Euclid Collaboration, A. Veropalumbo, M. Moresco +303
Higher-order correlation functions are firmly established as a fundamental tool for the statistical analysis of clustering in modern galaxy surveys. It was demonstrated that they g…
Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters
Euclid Collaboration, E. Tsaprazi, A. Fumagalli +274
The \textit{Euclid} satellite will deliver a catalogue of optically-selected galaxy clusters spanning from around deg in Data Release (DR) 1 to around deg…