Gravitational Lensing: Strong, Weak and Micro
By G. Meylan, P. Jetzer, P. North, P. Schneider, C. Kochanek, J. Wambsganss. 2006
622 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics
View Paper: https://www.semanticscholar.org/paper/0470f4f7899698b2f054800345bc71ce5fc48c12
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- T. Treu
- Rachel Mandelbaum
- P. J. Marshall
- H. Hoekstra
- Leon V. E. Koopmans
- M. Bartelmann
- T. Collett
- Risa Wechsler
In Atomic and Molecular Physics, and Optics
- P. J. Marshall
- Leon V. E. Koopmans
- T. Treu
- M. Auger
- Dominique Sluse
- Sherry H. Suyu
- C. Fassnacht
- Stefan Hilbert
Citations in the corpus
- Gravitational lensing (2010, background): “Many approaches to gravitational lensing exist, some of them heuristic, whereas others rather formal mathematically; see [358, 423, 425, 466, 492] for examples.”
- Galaxy Alignments: An Overview (2015, background): “A standard technical introduction to weak lensing is given in Bartelmann & Schneider (2001); see also Schneider (2006).”
- The Intrinsic Alignment of Galaxies and its Impact on Weak Gravitational Lensing in an Era of Precision Cosmology (2014, methodology): “The bispectrum due to nonlinear clustering is often estimated through the fitting formulae of Scoccimarro and Couchman (2001). The bispectrum is related to the power spectrum through second-order perturbation theory (Fry, 1984; Bernardeau et al.”
- DISSECTING THE GRAVITATIONAL LENS B1608+656. II. PRECISION MEASUREMENTS OF THE HUBBLE CONSTANT, SPATIAL CURVATURE, AND THE DARK ENERGY EQUATION OF STATE (2009, methodology): “Readable introductions to this type of analysis can be found in the books by Sivia (1996) and MacKay (2003); we use notation consistent with that in Paper I.”
- A Bayesian approach to strong lensing modelling of galaxy clusters (2007, methodology): “rare in current surveys, strong lensing events are expected to number as many as a few hundred thousand over the whole sky ( Cabanacet al2007). In order to fully exploit strong gravitational lensing events, one generally needs high resolution imaging coupled to deep spectroscopy to measure the redsh”
- Time delay cosmography (2016, background): “…2010; Treu et al. 2012; Jackson 2013, 2015; Treu and Ellis 2015) and not-so-recent (Blandford and Narayan 1992; Courbin et al. 2002; Kochanek et al. 2004; Falco 2005; Schneider et al. 2006) excellent reviews and textbooks (Schneider et al. 1992) for additional information and historical context.”