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1 is typical in other studies of extragalactic gravitational lensing.
2 reveals that he explored the possibility of gravitational lensing 3 years before completing his gene
4 f the large-scale structure in the universe, gravitational lensing, and the cosmic microwave backgrou
5 a factor of ten or more, as a consequence of gravitational lensing by galaxies along the line of sigh
8 surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficie
9 E(G), that combines measures of large-scale gravitational lensing, galaxy clustering and structure g
10 insights, including gravitational redshifts, gravitational lensing, gravitational waves, the Lense-Th
11 ng systems for astrophysical applications of gravitational lensing; in particular, they show structur
16 gravitational effects on stars and galaxies, gravitational lensing of light around these, and through
17 ence of the dark matter would be revealed by gravitational lensing of the light from an LMC star as t
19 ll 222/223 supercluster system from its weak gravitational lensing signal, both in a non-parametric m
20 2 was recently found using a method based on gravitational lensing, suggesting that the mass fraction
21 antifying image distortions caused by strong gravitational lensing-the formation of multiple images o
22 vity, and is most effectively probed through gravitational lensing: the deflection of light from dist
23 urements of the cosmic microwave background, gravitational lensing, type Ia supernovae, large-scale s
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