activity
20152026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 823 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026★ 1 cited

LenNet: Direct Detection and Localization of Strong Gravitational Lenses in Wide-Field Sky Survey Images

Pufan Liu, Hui Li, Ziqi Li +9

Strong gravitational lenses are invaluable tools for addressing fundamental questions in astrophysics, from the nature of dark matter to the expansion of the universe. While curren…

astro-ph.CO2024★ 550 cited

Euclid. I. Overview of the Euclid mission

Euclid Collaboration, Y. Mellier, Abdurro'uf +1134

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Eucl…

astro-ph.GA2017★ 219 cited

The third data release of the Kilo-Degree Survey and associated data products

J. T. A. de Jong, G. A. Verdoes Kleijn, T. Erben +40

The Kilo-Degree Survey (KiDS) is an ongoing optical wide-field imaging survey with the OmegaCAM camera at the VLT Survey Telescope. It aims to image 1500 square degrees in four fil…

astro-ph.GA2015

Early type galaxies and structural parameters from ESO public survey KiDS

N. Roy, N. R. Napolitano, F. La Barbera +5

The Kilo Degree survey (KiDS) is a large-scale optical imaging survey carried out with the VLT Survey Telescope (VST), which is the ideal tool for galaxy evolution studies. We expe…

astro-ph.GA2015★ 1 cited

Galaxy evolution within the Kilo-Degree Survey

C. Tortora, N. R. Napolitano, F. La Barbera +8

The ESO Public Kilo-Degree Survey (KiDS) is an optical wide-field imaging survey carried out with the VLT Survey Telescope and the OmegaCAM camera. KiDS will scan 1500 square degre…

astro-ph.GA2015★ 7 cited

Strong lens search in the ESO public Survey KiDS

N. R. Napolitano, G. Covone, N. Roy +10

We have started a systematic search of strong lens candidates in the ESO public survey KiDS based on the visual inspection of massive galaxies in the redshift range . As…