We present data products from the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS is based on the Wide component of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS). It encompasses 154 deg(2) of deep, optical, high-quality, sub-arcsecond imaging data in the five optical filters u*g(')r(')i(')z('). The scientific aims of the CFHTLenS team are weak gravitational lensing studies supported by photometric redshift estimates for the galaxies. This paper presents our data processing of the complete CFHTLenS data set. We were able to obtain a data set with very good image quality and high-quality astrometric and photometric calibration. Our external astrometric accuracy is between 60 and 70 mas with respect to Sloan Digi...
21 pages, 23 figures, 6 tablesWe present the first weak gravitational lensing analysis of the comple...
We present a finely-binned tomographic weak lensing analysis of the Canada-France-Hawaii Telescope L...
Light travelling through the Universe is deflected by the presence of mass, this effect will distort...
International audienceWe present data products from the Canada-France-Hawaii Telescope Lensing Surve...
We present data products from the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS...
We present data products from the Canada\u2013France\u2013Hawaii Telescope Lensing Survey (CFHTLenS)...
We present data products from the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS...
International audienceWe present the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS) that a...
We present the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS) that accurately determines a...
The Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS) comprises deep multi-colour (u*g'r'i'z'...
International audienceHere we present the results of various approaches to measure accurate colours ...
Here we present the results of various approaches to measure accurate colours and photometric redshi...
We present the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS) that accurately determines a...
We present the first weak gravitational lensing analysis of the completed Canada-France-Hawaii Teles...
We present the Red-sequence Cluster Lensing Survey (RCSLenS), an application of the methods develope...
21 pages, 23 figures, 6 tablesWe present the first weak gravitational lensing analysis of the comple...
We present a finely-binned tomographic weak lensing analysis of the Canada-France-Hawaii Telescope L...
Light travelling through the Universe is deflected by the presence of mass, this effect will distort...
International audienceWe present data products from the Canada-France-Hawaii Telescope Lensing Surve...
We present data products from the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS...
We present data products from the Canada\u2013France\u2013Hawaii Telescope Lensing Survey (CFHTLenS)...
We present data products from the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS...
International audienceWe present the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS) that a...
We present the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS) that accurately determines a...
The Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS) comprises deep multi-colour (u*g'r'i'z'...
International audienceHere we present the results of various approaches to measure accurate colours ...
Here we present the results of various approaches to measure accurate colours and photometric redshi...
We present the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS) that accurately determines a...
We present the first weak gravitational lensing analysis of the completed Canada-France-Hawaii Teles...
We present the Red-sequence Cluster Lensing Survey (RCSLenS), an application of the methods develope...
21 pages, 23 figures, 6 tablesWe present the first weak gravitational lensing analysis of the comple...
We present a finely-binned tomographic weak lensing analysis of the Canada-France-Hawaii Telescope L...
Light travelling through the Universe is deflected by the presence of mass, this effect will distort...