The Kilo-Degree Survey
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).
attn: J. T. A. de Jong
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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.
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.
KiDS Data Release 3 available
10 Oct 2016
The third public data release (DR3) of KiDS is as now available. Adding 292 survey tiles to the previous releases, DR3 brings the total number of released tiles to 440. New features in the DR3 multi-band catalog, which covers the combined survey area of DR1, DR2 and DR3, are Gaussian Aperture and PSF (GAaP) photometry, survey photometric homogenization, and photometric redshifts. Further details, the release notes, and data access information can be found on the DR3 website.
KiDS measures cosmic shear from 15 million galaxies
16 June 2016
Based on 450 square degrees of imaging, we have obtained the first cosmological parameter constraints from KiDS. The main result is shown in the Figure, in the form of constraints on the σ8 - Ωmatter plane. Interestingly, and in common with many other low-redshift probes, the best-fit values show a discrepancy with the expectation from Planck cosmology. Further studies are underway.
Constraints in the Ωm vs. σ8 plane from KiDS-450 cosmic shear tomography (green) in comparison to CFHTLenS (gray), WMAP9+ACT+SPT (blue), and Planck 2015 (orange).
Dutch broadcaster VPRO interviews Margot Brouwer
18 May 2016
Dutch broadcasting corporation VPRO interviewed Leiden University Phd student Margot Brouwer about her work on KiDS. The article, which is only available in Dutch, has been published in the VPRO tv guide, but can also be downloaded below. On Thursday May 19th at 19:20 CEST, a related documentary focused on the nature of Dark Matter will be broadcast on Dutch public tv station NPO2.
First science results from KiDS published
6 Jul 2015
Today the first scientific results from the Kilo-Degree Survey have been published. Among the first batch of papers are early weak gravitational lensing analyses, demonstrating the power of the superb image quality of KiDS for this type of research. Other results presented include the discovery of four high-redshift quasars, a sample of super-compact massive galaxies, and a catalog of photometric redshift based on machine learning techniques. Links to the papers are provided on the Papers page, and press releases highlighting these first results can be found via the Press releases page.
Animated gif of a group of galaxies, with and without the invisible dark matter rendered in pink. Credit: Kilo-Degree Survey Collaboration/A. Tudorica & C. Heymans/ESO
Lensing catalogs available
6 Jul 2015
With the announcement of the first weak lensing analyses using KiDS data, the weak lensing shear catalogs are also released. The area covered is the overlap of the combined data set of the first two KiDS public data releases with the equatorial regions covered by the GAMA survey. Shear measurements are made using a dedicated pipeline using THELI and Lensfit, while the included photometry and photometric redshifts are derived from the DR1/2 coadded images using image gaussianization and Gaussian-weighted aperture photometry.
Please visit the Lensing catalogs page for details and data access.
KiDS Data Release 2 available
18 Feb 2015
The second public data release of KiDS (KiDS-ESO-DR2) is available. It contains calibrated, stacked images and their weights, masks and single-band source lists for 98 square degrees, as well as a multi-band source catalog encompassing the 150 square degrees of the first two KiDS data releases combined. All data are available via the ESO archive facility, as well as via the AstroWISE Information System.
Please visit the KiDS Data Release 2 pages for details and data access.