activity
20132026
most citedEuclid. III. The NISP Instrument

114 citations · 1.8k across the 214 of their papers we have counts for

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Showing 2022Show all

12 papers · 1 filter

astro-ph.CO2022★ 14 cited

Modelling the next-to-leading order matter three-point correlation function using FFTLog

M. Guidi, A. Veropalumbo, E. Branchini +2

The study of higher-order statistics, particularly three-point statistics, of the Large Scale Structure (LSS) of the Universe provides us with unique information on the biasing rel…

astro-ph.CO2022

Euclid preparation. XXVII. Covariance model validation for the 2-point correlation function of galaxy clusters

Euclid Collaboration, A. Fumagalli, A. Saro +191

Aims. We validate a semi-analytical model for the covariance of real-space 2-point correlation function of galaxy clusters. Methods. Using 1000 PINOCCHIO light cones mimicking the…

astro-ph.GA2022★ 26 cited

Euclid preparation. XXV. The Euclid Morphology Challenge -- Towards model-fitting photometry for billions of galaxies

Euclid Collaboration, E. Merlin, M. Castellano +218

The ESA Euclid mission will provide high-quality imaging for about 1.5 billion galaxies. A software pipeline to automatically process and analyse such a huge amount of data in real…

astro-ph.CO2022

Euclid preparation. XXIV. Calibration of the halo mass function in CDM cosmologies

Euclid Collaboration, T. Castro, A. Fumagalli +179

Euclid's photometric galaxy cluster survey has the potential to be a very competitive cosmological probe. The main cosmological probe with observations of clusters is their number…

astro-ph.CO2022★ 9 cited

Testing General Relativity: new measurements of gravitational redshift in galaxy clusters

D. Rosselli, F. Marulli, A. Veropalumbo +2

The peculiar velocity distribution of cluster member galaxies provides a powerful tool to directly investigate the gravitational potentials within galaxy clusters and to test the g…

astro-ph.CO2022★ 15 cited

Fitting covariance matrix models to simulations

Alessandra Fumagalli, Matteo Biagetti, Alexandro Saro +4

Data analysis in cosmology requires reliable covariance matrices. Covariance matrices derived from numerical simulations often require a very large number of realizations to be acc…

astro-ph.CO2022★ 12 cited

Euclid preparation: XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data release

Euclid Collaboration, R. Saglia, S. De Nicola +183

The Complete Calibration of the Color-Redshift Relation survey (C3R2) is a spectroscopic programme designed to empirically calibrate the galaxy color-redshift relation to the Eucli…

astro-ph.CO2022★ 8 cited

The halo 3-point correlation function: a methodological analysis

A. Veropalumbo, A. Binetti, E. Branchini +5

We measure the 3PCF of 300 halo catalogs from the Minerva simulations covering a total volume of . Each 3PCF measurement includes all possible triangul…

astro-ph.CO2022★ 58 cited

Euclid: Cosmological forecasts from the void size function

S. Contarini, G. Verza, A. Pisani +123

The Euclid mission with its spectroscopic galaxy survey covering a sky area over in the redshift range will provide a sample of tens o…

astro-ph.GA2022★ 1 cited

Tracing the environmental history of observed galaxies via extended fast action minimization method

Elena Sarpa, Alessia Longobardi, Katarina Kraljic +2

We present a novel application of the extended Fast Action Minimization method (eFAM) aimed at assessing the role of the environment in shaping galaxy evolution. We validate our ap…

astro-ph.CO2022★ 37 cited

AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering

G. F. Lesci, L. Nanni, F. Marulli +13

We analysed the clustering of a photometric sample of galaxy clusters selected from the Third Data Release of the Kilo-Degree Survey, focusing on the redshift-space two-point corre…

astro-ph.CO2022★ 24 cited

New constraints on primordial features from the galaxy two-point correlation function

Mario Ballardini, Fabio Finelli, Federico Marulli +2

Features in the primordial power spectrum represent the imprinted signal in the density perturbations of the physics and evolution of the early Universe. A measurement of such sign…