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KiDS

The Kilo-Degree Survey (KiDS) is an astronomical wide-field survey. Designed as a weak lensing shear tomography survey, the main science drivers are to map the mass distribution in the universe and to constrain the equation-of-state of dark energy.

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KiDS | kids.strw.leidenuniv.nl Reviews
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DESCRIPTION
The Kilo-Degree Survey (KiDS) is an astronomical wide-field survey. Designed as a weak lensing shear tomography survey, the main science drivers are to map the mass distribution in the universe and to constrain the equation-of-state of dark energy.
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1 Kilo Degree Survey
2 KiDS
3 survey
4 kids survey
5 VST
6 cosmology
7 lensing
8 omegacam
9 dark energy
10 astronomy
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KiDS | kids.strw.leidenuniv.nl Reviews

https://kids.strw.leidenuniv.nl

The Kilo-Degree Survey (KiDS) is an astronomical wide-field survey. Designed as a weak lensing shear tomography survey, the main science drivers are to map the mass distribution in the universe and to constrain the equation-of-state of dark energy.

INTERNAL PAGES

kids.strw.leidenuniv.nl kids.strw.leidenuniv.nl
1

KiDS

http://kids.strw.leidenuniv.nl/availability.php

As KiDS is an ESO Public Survey, all KiDS data will be publicly released. Basic data products will include astrometrically and photometrically calibrated coadded imaging, and single-band and multi-band source lists. On longer timescales KiDS is also committed to provide higher-level data products, which may include Gaussianized images, or value-added catalogues with PSF-matched multi-band photometry or source analysis results. KiDS-450 paper and data access. The second public data release of KiDS (KiDS-E...

2

KiDS

http://kids.strw.leidenuniv.nl/processing.php

Within the KiDS team two data processing chains are used. The Astro-WISE pipeline is used as the main tool for data processing, data management, and monitoring of the telescope and instrument. This pipeline is also used to produce the public survey data products. Secondly, a lensing-optimized processing chain consisting of the THELI data reduction pipeline and the LensFit shape measurement code are used for specific weak lensing analyses. The cosmic shear application of KiDS requires highly specialized a...

3

KiDS

http://kids.strw.leidenuniv.nl/pressreleases.php

Huge new survey to shine light on dark matter. July 9th, 2015. First images from the VLT Survey Telescope. June 8th, 2011. Website design: Fenids Webdesign.

4

KiDS

http://kids.strw.leidenuniv.nl/progress.php

Official KiDS observations commenced in semester P88, which for VST observations started on October 15th 2011. The figures below show per filter which tiles have been successfully observed and ingested into the Astro-WISE data reduction system. Website design: Fenids Webdesign.

5

KiDS

http://kids.strw.leidenuniv.nl/links.php

European Southern Observatory (ESO). VLT Survey Telescope (VST). OmegaCAM: the VST camera. Galaxy And Mass Assembly. 2dF Galaxy Redshift Survey. Sloan Digital Sky Survey. Website design: Fenids Webdesign.

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gama-survey.org gama-survey.org

GAMA | Galaxy And Mass Assembly

http://www.gama-survey.org/dr2

GAMA Data Release 2. The second GAMA data release (DR2) provides AAT/AAOmega spectra, redshifts and a wealth of ancillary information for 72,225 objects from the first phase of the GAMA survey (2008 - 2010, usually referred to as GAMA I). The DR2 web pages describe the data included in this release, and provide access to an SQL database as well as to the actual data (spectra and catalogues). If you are using GAMA DR2 data in a publication then please cite the DR2 paper (Liske et al. 2015). Minus;1 - 3.

gama-survey.org gama-survey.org

GAMA | Galaxy And Mass Assembly

http://www.gama-survey.org/dr1

GAMA papers on ADS. Papers referring to GAMA on arXiv. The links below constitute GAMA's first data release. Which is described in Driver et al (2011). From this website you can access the entire GAMA first data release. We have provided a MySQL tool. We have provided tools. For inspecting our mosaics, and for extracting postage stamps from them. They provide a simple interface, allowing quick searching for single objects or near-position searches in the GAMA data.

m2teamsoftware.it m2teamsoftware.it

I.N.A.F. Astronomical Observatory of Capodimonte

http://m2teamsoftware.it/vst

Description of the facility. VST in a nutshell. The VLT Survey Telescope, dubbed as VST, is a wide-field optical imager with a 2.61 m aperture conceived for the superb environment of the. It operates from the UV to the I band, preserving, within a corrected field of view of 1 x. 1 , the seeing conditions achievable at the Cerro Paranal site. The telescope is equipped with just one focal plane instrument, OmegaCAM. A large format (16k x. And the Capodimonte Astronomical Observatory ( OAC. The survey aims ...

kiaa-clusters.voxcharta.org kiaa-clusters.voxcharta.org

Earth and Planetary « Vox Charta

http://kiaa-clusters.voxcharta.org/category/astro-ph/earth-planetary-astro-ph

ArXiv discussions for 389 institutions. Including Stockholm Galaxy Group. Argelander-Institut fur Astronomie (AIfA). Brandenberger 's Group Meeting. CEA Saclay Cosmology and Galaxy Evolution. CEA Saclay High Energy. Cardiff Physics and Astronomy. Center for Computational Astrophysics. Centro Nacional de Biotecnologia. EA Milne Centre for Astrophysics. ECAP - Universitaet Erlangen-Nuremberg. Florida A&M University Physics. GCON - Cosmology Group of the National Observatory. GRBs in several institutions.

astro-wise.org astro-wise.org

Astro-WISE - Supported data sources

http://www.astro-wise.org/portal/aw_datasources.shtml

Data and Software Viewing Grid. Here you can find quick links to different subsets of data in our database. Find data for the OMEGACAM instrument. Find data for the VIRCAM instrument. Find data for LOFAR. Find data for the DECAM instrument. Find data for the WFI instrument. Find data for the MegaCAM instrument. Wide-Field Camera on the Isaac Newton Telescope at La Palma. Suprime-Cam data from the Subaru telescope on Mauna Kea, Hawaii. Find data for the KIDS project. Find data for the ATLAS project.

cfhtlens.org cfhtlens.org

The Canada France Hawaii Lensing Survey | CFHTLenS

http://www.cfhtlens.org/public/canada-france-hawaii-lensing-survey

The intricate cosmic web of dark matter and galaxies spanning more than one billion light years. The pink-yellow plumes seen with gravitational lensing show us where the dark matter is. The Canada France Hawaii Lensing Survey. Did you know that less than 4% of our Universe is made up of regular matter - the type that makes up the Earth, the planets and the stars? The rest is 'dark' and invisible, but we know that it is there through its effects on the regular matter that we. Welcome to our website!

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kids.strw.leidenuniv.nl kids.strw.leidenuniv.nl

KiDS

KiDS: the Kilo Degree Survey. KiDS, the Kilo-Degree Survey, is a new, large-scale 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 filters (u, g, r, i). If you want to know even more about the project! News: First science results from KiDS published. Shear measurements are m...

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