For you to get the most out of this website. We have divided the content in to two sections:. Astronomers reach new frontiers of dark matter: see dark matter mapped over the largest scales ever observed, learn about the Dark Universe and the technique gravitational lensing that we use to see the invisible! Access CFHTLenS journal publications, the CFHTLenS data release, public software and general survey information. Site by Ben Dugdale.
http://www.cfhtlens.org/
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Welcome | CFHTLenS | cfhtlens.org Reviews
https://cfhtlens.org
For you to get the most out of this website. We have divided the content in to two sections:. Astronomers reach new frontiers of dark matter: see dark matter mapped over the largest scales ever observed, learn about the Dark Universe and the technique gravitational lensing that we use to see the invisible! Access CFHTLenS journal publications, the CFHTLenS data release, public software and general survey information. Site by Ben Dugdale.
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!
The CFHT Lensing Survey | CFHTLenS
http://www.cfhtlens.org/astronomers/content-suitable-astronomers
The Canada-France-Hawaii Telescope on Mauna Kea, Hawaii. CFHTLenS uses data imaged by the CFHT Legacy Survey which completed observations in early 2009. Image credit J.-C. Cuillandre. The CFHT Lensing Survey. Welcome to the Astronomer section of the website for the Canada-France Hawaii Telescope Lensing Survey: CFHTLenS. Access the CFHTLenS Shear and Photometric Redshift catalogues here. CFHTLenS is a 154 square degree multi-colour optical survey in ugriz. And Heymans et al 2012. Gaussianised Photometry ...
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msslastro | Late Universe
https://lateuniverse.wordpress.com/author/msslastro
Explorations in survey cosmology, theoretical physics, signal processing, and Bayesian inference. Science on the Sphere. How rich is a galaxy cluster? October 13, 2014. Post by Tom Kitching. In a recent paper http:/ arxiv.org/abs/1409.3571. Lead by Jes Ford http:/ www.phas.ubc.ca/ jesford/Welcome.html. The mass- richness relation of galaxy clusters was investigating using data from the CFHTLenS survey. Chance that we have detected a weak lensing signal behind these clusters and groups! The main result in...
Martin Kilbinger | CosmoStat
http://www.cosmostat.org/people/kilbinger
An AIM laboratory @CEA Saclay. Joint Planck PR1 WMAP CMB Map. Joint Planck PR2 WMAP CMB map. Galaxy colour component separation. PSF estimation and images restoration. Jean-Luc Starck, Head of CosmoStat. Jerome Bobin, co-head of CosmoStat. Sparse BSS with GMCALab. Non-negative matrix factorization with nGMCA. WMAP9 Point Source Free Map. Euclid CEA - IAP meetings. Euclid WL 2p-stat meeting. Machine learning day at SAp. RAS discussion meeting on Cosmology with Maps. How to get to SAp. Which is part of IRFU.
KiDS
http://kids.strw.leidenuniv.nl/overview.php
KiDS will survey two areas of extragalactic sky, some 750 square degrees each, in four filters (u,g,r,i). In parallel, the companion VIKING project on the neighbouring VISTA telescope will cover the same area in five near-infrared bands: Z,Y,J,H,K. The integration times (see technical specifications. Page) are chosen so that the survey will reach a median redshift of 0.7. The lay-out of the survey fields is chosen to overlap with previous, publicly available huge galaxy redshift surveys ( 2dF. Figure 1: ...
Points to Three Points | Late Universe
https://lateuniverse.wordpress.com/2014/05/30/points-to-three-points
Explorations in survey cosmology, theoretical physics, signal processing, and Bayesian inference. Science on the Sphere. Science on the Sphere. Combining information over 13 billion years of time →. Points to Three Points. May 30, 2014. Post by Tom Kitching, MSSL. In a recent paper. Led by collaborator Dr Liping Fu the CFHTLenS. Excess probability that any pair of galaxies (separated by a particular angular distance) are aligned. And can be used to measure cosmological parameters, which is why we are int...
abril 2014 - Lukay: Astrofísica Chilena
http://lukayastro.blogspot.com/2014_04_01_archive.html
Divulgando publicaciones en astronomía, astrofísica y cosmología lideradas por chilenos. Ivan Lacerna: Galaxias centrales en diferentes ambientes. Lunes, 28 de abril de 2014. Usando catálogos extraídos del Sloan Digital Sky Survey ( SDSS. Central galaxies in different environments: Do they have similar properties? Ivan Lacerna, Aldo Rodriguez-Puebla, Vladimir Avila-Reese and Hector M. Hernandez-Toledo. Aceptado para su publicación en ApJ. 160;ArXiv: 1311.6473. Publicado por Lukay Astro. Cuando anuncies t...
The power of three | Late Universe
https://lateuniverse.wordpress.com/2014/01/28/the-power-of-three
Explorations in survey cosmology, theoretical physics, signal processing, and Bayesian inference. Science on the Sphere. Wavelets for studying the large-scale structure (LSS) of the Universe →. The power of three. January 28, 2014. Post by Tom Kitching. Today a paper of mine that I have been working on for the last few years was posted to the arXiv. What is 3D cosmic shear? We also see galaxies in a 3. Dimension are not only distant in a space but also distant in time. The 3D distribution of galaxies...
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.
Projects | CosmoStat
http://www.cosmostat.org/project
An AIM laboratory @CEA Saclay. Joint Planck PR1 WMAP CMB Map. Joint Planck PR2 WMAP CMB map. Galaxy colour component separation. PSF estimation and images restoration. Jean-Luc Starck, Head of CosmoStat. Jerome Bobin, co-head of CosmoStat. Sparse BSS with GMCALab. Non-negative matrix factorization with nGMCA. WMAP9 Point Source Free Map. Euclid CEA - IAP meetings. Euclid WL 2p-stat meeting. Machine learning day at SAp. RAS discussion meeting on Cosmology with Maps. How to get to SAp. Develop tools for an...
Celebrating the Persian New Year at MSSL | mssl astro
https://msslastro.wordpress.com/2015/03/20/celebrating-the-persian-new-year-at-mssl
Mullard Space Science Laboratory Astronomy Blog. Celebrating the Persian New Year at MSSL. March 20, 2015. I am Paniez Paykari, a new postdoctoral researcher at MSSL-UCL. I am a cosmologist and since joining. The Astro group at MSSL in February, I have been. Ensing (WL). My previous work was mostly focused on the cosmic microwave background (CMB). I work with Tom Kitching, co-leader of the Euclid. Weak Lensing Science Working Group, and the leader of the CFHTLenS. Familiar with me and my research. The.
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Welcome | CFHTLenS
For you to get the most out of this website. We have divided the content in to two sections:. Astronomers reach new frontiers of dark matter: see dark matter mapped over the largest scales ever observed, learn about the Dark Universe and the technique gravitational lensing that we use to see the invisible! Access CFHTLenS journal publications, the CFHTLenS data release, public software and general survey information. Site by Ben Dugdale.
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