The Kilo-Degree Survey

The VLT Survey Telescope at sunset at Paranal Observatory

KiDS, the Kilo-Degree Survey, is a large optical imaging survey in the Southern sky, designed to tackle some of the most fundamental questions of cosmology and galaxy formation of today. Using the VLT Survey Telescope (VST), located at the ESO Paranal Observatory, KiDS will map 1500 square degrees of the night sky in four broad-band filters (u, g, r, i).

Survey overview
Scientific goals

Contact

Email:

kids_at_strw.leidenuniv.nl

Postal address:

KiDS survey
attn: J. T. A. de Jong
Sterrewacht Leiden
P.O. Box 9513
NL-2300 RA Leiden
The Netherlands

Finding galaxy clusters in KiDS

7 Feb 2017

The first galaxy cluster catalog from KiDS, based on the DR2 data set, has been published in Radovich et al. (2017, A&A, 598, A107). Accompanying the paper is a catalog of 1585 candidate clusters, extending to a redshift of 0.7, and shown to be 85% complete, with an estimated purity of 80%. This catalog can be downloaded from the cluster catalog webpage linked below. The tools (developed by F. Bellagamba, M. Maturi and M. Roncarelli) that have been used to harvest the KiDS data for galaxy clusters and presented in this paper, have also been selected for use by the upcoming ESA Euclid satellite mission.

Paper on A&A website
DR2 cluster catalog webpage

  

Central 2 arcsecond region of the cluster Abell 1411, one of the rich clusters present in the KiDS DR2 area. This color image was made from KiDS u-, g- and r-band data and shows the Brightest Cluster Galaxy, indicated by the green circle; the red circle shows the cluster center reported in the Abell catalog.

KiDS goes to the Galaxy Zoo

1 Feb 2017

Images from the Kilo-Degree Survey (KiDS) are now included in the Galaxy Zoo citizen science project, where anyone can help classify galaxies and contribute to our astronomical knowledge. Currently, for over 11,000 galaxies, selected based on a galaxy catalog from the GAMA survey, color images from KiDS g-, r- and i-band data are available. This data set will later on be extended step-wise to over 40,000 galaxies. The high quality KiDS images will allow us to study the very faintest structures within galaxies, as well as more accurately classify features which may have been missed before.

Galaxy Zoo
Blog post: New images for Galaxy Zoo from GAMA-KiDS!

KiDS-450 Weak lensing shear catalog released

3 Jan 2017

The weak lensing shear catalog for the KiDS-450 / DR3 data set, covering 454 KiDS survey tiles is now publicly available. This data set serves as the basis for the cosmic shear analysis presented in Hildebrandt & Viola et al. (2017) and various more scientific analyses currently in preparation. Available both via ESO and CADC, the catalog provides accurate shear measurements and photometric redshifts for over 15 million galaxies.

KiDS-450 Weak Lensing catalog

Dark matter may be smoother than expected

7 Dec 2016

Analysis of 450 square degrees of the Kilo-Degree Survey (KiDS), made with ESO's VLT Survey Telescope in Chile, suggests that dark matter may be less dense and more smoothly distributed throughout space than previously thought. An international team studied how the light from about 15 million distant galaxies was affected by the gravitational influence of matter on the largest scales in the Universe. The results appear to be in disagreement with earlier results from the Planck satellite. Press releases highlighting these results can be found via the Press releases page.

  

Dark matter map of KiDS survey region (region G15). Credit: Kilo-Degree Survey Collaboration/H. Hildebrandt & B. Giblin/ESO.