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1 rs magnify background objects through strong gravitational lensing.
2 ming caustics analogous to those produced by gravitational lensing.
3 ng, of a distant galaxy that is magnified by gravitational lensing.
4 is typical in other studies of extragalactic gravitational lensing.
5 reveals that he explored the possibility of gravitational lensing 3 years before completing his gene
7 f the large-scale structure in the universe, gravitational lensing, and the cosmic microwave backgrou
9 appeared in multiple images produced through gravitational lensing by a massive foreground galaxy clu
10 a factor of ten or more, as a consequence of gravitational lensing by galaxies along the line of sigh
13 surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficie
15 E(G), that combines measures of large-scale gravitational lensing, galaxy clustering and structure g
16 insights, including gravitational redshifts, gravitational lensing, gravitational waves, the Lense-Th
17 ng systems for astrophysical applications of gravitational lensing; in particular, they show structur
23 gravitational effects on stars and galaxies, gravitational lensing of light around these, and through
24 ence of the dark matter would be revealed by gravitational lensing of the light from an LMC star as t
26 of the James Webb Space Telescope (JWST) and gravitational lensing shows that this ultra-faint galaxy
27 ll 222/223 supercluster system from its weak gravitational lensing signal, both in a non-parametric m
28 2 was recently found using a method based on gravitational lensing, suggesting that the mass fraction
29 antifying image distortions caused by strong gravitational lensing-the formation of multiple images o
30 vity, and is most effectively probed through gravitational lensing: the deflection of light from dist
31 cope (JWST) combined with magnification from gravitational lensing, these low-mass galaxies can not o
32 urements of the cosmic microwave background, gravitational lensing, type Ia supernovae, large-scale s