Weak Gravitational Lensing

By S. Pires, Jean-Luc Starck, A. Leonard, Alexandre Refregier. 2012

559 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d79ae273ffe82fe6d668eceeed90abfb11ebc9b8

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In Astronomy and Astrophysics

Citations in the corpus

DeepCMB: Lensing Reconstruction of the Cosmic Microwave Background with Deep Neural Networks (2018, background): “For reviews, see Dodelson (2003); Lewis and Challinor (2006).”
General Relativity and Cosmology: Unsolved Questions and Future Directions (2016, background): “Although the theory of cosmic shear had been worked out from the 1960s to the early 1990s [242], the first detection had to await the development of instruments sensitive enough to make the required observations, and image analysis software to accurately correct for unwanted effects when measuring t”
DeepSphere: Efficient spherical Convolutional Neural Network with HEALPix sampling for cosmological applications (2018, methodology): “These kind of maps can be created using the gravitational lensing technique [see 29, for review].”
Dark matter direct-detection experiments (2015, background): “Measurements of the Lyman−α forest [12][13] and weak lensing [14][15] confirm the cosmic structure considering not only galaxies and gas clouds but also non-luminous and non-baryonic matter.”
Transformation Importance with Applications to Cosmology (2020, background): “a galaxy survey), these mass maps are obtained by measuring the distortion of distant galaxies caused by the deflection of light by the mass between the galaxy and the observer [17].”
Gravitational lensing (2010, background): “Weak gravitational lensing by large-scale structures is covered by several dedicated reviews, highlighting different aspects of this rich and quickly developing subject [320, 27, 205, 322, 399, 201, 355].”
Galaxy Alignments: Observations and Impact on Cosmology (2015, background): “See Bartelmann & Schneider (2001); Hoekstra & Jain (2008); Munshi et al. (2008); Bartelmann (2010) for general reviews of weak lensing.”
Gravitational Lensing in Presence of Plasma: Strong Lens Systems, Black Hole Lensing and Shadow (2017, background): “Now gravitational lensing is a powerful astrophysical tool for investigations of distant objects, a distribution of dark matter and large scale structure, the cosmic microwave background, discovery of planet and checking of the General Relativity, see some reviews, classical and interesting recent w”
The Intrinsic Alignment of Galaxies and its Impact on Weak Gravitational Lensing in an Era of Precision Cosmology (2014, methodology): “2004); Ishak (2005); Ishak and Hirata (2005)). We will brieﬂy mention some of these here, but recommend more extensive reviews on gravitational lensing (e.g., Schneider et al. (1992); Mellier (1999); Bartelmann and Schneider (2001); Wittman (2002); Refregier (2003b); van Waerbeke and Mellier (2003);”
Primordial non-Gaussianity from the large-scale structure (2010, background): “Weak lensing is another direct probe of the dark matter, although we can only observe it in projection along the line of sight [77].”
Galaxy Masses: A Review (2013, methodology): “2010; Battaglia et al. 2011; Simon et al. 2011). We refer the reader to the detailed review by Battaglia et al. (2013). An example of this method is shown in Figure 18 for the Sculptor dwarf spheroidal galaxy, studied in detail by Battaglia et al. (2008), who fit the PPS assuming Gaussian LOS veloci”
f(R) Theories (2010, background): “Then the convergence has the same power spectrum as Pκ, which is given by [66, 601]”