activity
19992025
most citedThe first and second data releases of the Kilo-Degree Survey

295 citations · 1.5k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.GA2025★ 44 cited

The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields

Angus H. Wright, Konrad Kuijken, Hendrik Hildebrandt +51

We present the final data release of the Kilo-Degree Survey (KiDS-DR5), a public European Southern Observatory (ESO) wide-field imaging survey optimised for weak gravitational lens…

astro-ph.CO2024★ 2 cited

Where do X-ray low surface brightness clusters sit with respect to filaments?

S. Zarattini, S. Andreon, E. Puddu

The aim of this work is to study the position of gas-rich and gas-poor galaxy clusters within the large-scale structure and, in particular, their distance to filaments. Our sample…

astro-ph.CO2024★ 16 cited

AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing

Carlo Giocoli, Lorenzo Palmucci, Giorgio F. Lesci +13

Context. Weak gravitational lensing offers a powerful method to investigate the projected matter density distribution within galaxy clusters, granting crucial insights into the bro…

astro-ph.CO2023★ 4 cited

AMICO galaxy clusters in KiDS-DR3: constraints on CDM from extreme value statistics

Valerio Busillo, Giovanni Covone, Mauro Sereno +11

We constrain the CDM cosmological parameter by applying the extreme value statistics for galaxy cluster mass on the AMICO KiDS-DR3 catalog. We sample the posterior distr…

astro-ph.CO2023★ 8 cited

Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps

Denis Tramonte, Yin-Zhe Ma, Ziang Yan +11

We provide novel constraints on the parameters defining the universal pressure profile (UPP) within clusters of galaxies, and explore their dependence on the cluster mass and redsh…

astro-ph.CO2022★ 18 cited

Simulation view of galaxy clusters with low X-ray surface brightness

Antonio Ragagnin, Stefano Andreon, Emanuella Puddu

X-ray selected samples are known to miss galaxy clusters that are gas poor and have a low surface brightness. This is different for the optically selected samples such as the X-ray…