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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2015, Volume 454, Issue 2, pp. 1221 - 1221
One of the most powerful techniques to study the dark sector of the Universe is weak gravitational lensing. In practice, to infer the reduced shear, weak... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2015, Volume 454, Issue 2, p. 1221
  One of the most powerful techniques to study the dark sector of the Universe is weak gravitational lensing. In practice, to infer the reduced shear, weak... 
Universe | Probability distribution | Star & galaxy formation | Bayesian analysis | Gravity
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2015, Volume 454, Issue 2, pp. 1221 - 1221
One of the most powerful techniques to study the dark sector of the Universe is weak gravitational lensing. In practice, to infer the reduced shear, weak... 
Ellipticity | Reduction | Gravitational lenses | Shear | Noise | Noise reduction | Mathematical models | Photometry
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 459, Issue 1, p. 971
  There is currently a discrepancy in the measured value of the amplitude of matter clustering, parametrized using s8, inferred from galaxy weak lensing, and... 
Astrophysics | Dark matter | Simulation | Cosmic microwave background temperature | Neutrinos | Star & galaxy formation | Gravity
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 459, Issue 1, pp. 971 - 971
There is currently a discrepancy in the measured value of the amplitude of matter clustering, parametrized using s8, inferred from galaxy weak lensing, and... 
Red shift | Shear | Feedback | Neutrinos | Cosmic microwave background | Mathematical models | Photometry | Baryons
Journal Article
by Amendola, Luca and Appleby, Stephen and Avgoustidis, Anastasios and Bacon, David and Baker, Tessa and Baldi, Marco and Bartolo, Nicola and Blanchard, Alain and Bonvin, Camille and Borgani, Stefano and Branchini, Enzo and Burrage, Clare and Camera, Stefano and Carbone, Carmelita and Casarini, Luciano and Cropper, Mark and de Rham, Claudia and Dietrich, Jörg P and Di Porto, Cinzia and Durrer, Ruth and Ealet, Anne and Ferreira, Pedro G and Finelli, Fabio and García-Bellido, Juan and Giannantonio, Tommaso and Guzzo, Luigi and Heavens, Alan and Heisenberg, Lavinia and Heymans, Catherine and Hoekstra, Henk and Hollenstein, Lukas and Holmes, Rory and Hwang, Zhiqi and Jahnke, Knud and Kitching, Thomas D and Koivisto, Tomi and Kunz, Martin and La Vacca, Giuseppe and Linder, Eric and March, Marisa and Marra, Valerio and Martins, Carlos and Majerotto, Elisabetta and Markovic, Dida and Marsh, David and Marulli, Federico and Massey, Richard and Mellier, Yannick and Montanari, Francesco and Mota, David F and Nunes, Nelson J and Percival, Will and Pettorino, Valeria and Porciani, Cristiano and Quercellini, Claudia and Read, Justin and Rinaldi, Massimiliano and Sapone, Domenico and Sawicki, Ignacy and Scaramella, Roberto and Skordis, Constantinos and Simpson, Fergus and Taylor, Andy and Thomas, Shaun and Trotta, Roberto and Verde, Licia and Vernizzi, Filippo and Vollmer, Adrian and Wang, Yun and Weller, Jochen and Zlosnik, Tom and Euclid Theory Working Grp and Euclid Theory Working Group and The Euclid Theory Working Group and Case Western Reserve Univ., Cleveland, OH (United States) and Nordic Institute for Theoretical Physics NORDITA and KTH and Centra
Living Reviews in Relativity, ISSN 2367-3613, 12/2018, Volume 21, Issue 1, pp. 1 - 345
Journal Article