activity
20222026
most citedAMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis

20 citations · 42 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2026

AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function

G. F. Lesci, C. Giocoli, F. Marulli +9

We present the splashback radius analysis of the Adaptive Matched Identifier of Clustered Objects (AMICO) galaxy cluster sample in the fourth data release of the Kilo Degree Survey…

astro-ph.CO2025★ 4 cited

AMICO galaxy clusters in KiDS-1000: cosmological sample

M. Maturi, M. Radovich, L. Moscardini +12

Context. Galaxy clusters provide key insights into cosmic structure formation, galaxy formation and are essential for cosmological studies. Aims. We present a catalog of galaxy clu…

astro-ph.CO2025★ 5 cited

AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing

G. F. Lesci, F. Marulli, L. Moscardini +14

We present the joint modelling of weak-lensing and count measurements of the galaxy clusters detected with the AMICO code, in the fourth data release of the Kilo Degree Survey (KiD…

astro-ph.CO2023★ 13 cited

AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function

M. Romanello, F. Marulli, L. Moscardini +14

We study the tomographic clustering properties of the photometric cluster catalogue derived from the Third Data Release of the Kilo Degree Survey, focusing on the angular correlati…

astro-ph.CO2022★ 20 cited

AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis

Lorenzo Ingoglia, Giovanni Covone, Mauro Sereno +19

Galaxy clusters are biased tracers of the underlying matter density field. At very large radii beyond about 10 Mpc/\textit{h}, the shear profile shows evidence of a second-halo ter…