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Thus, clusters of galaxies with masses M ∼ 1015M⊙ at cosmological distances can result in Einstein rings with angular radii tens of arcseconds.
2012, Arlie O. Petters, Harold Levine, Joachim Wambsganss, Singularity Theory and Gravitational Lensing, Springer, page 155:
The many constraints that the images of Einstein rings provide, allow us to determine the slope of the mass distribution in the lensing galaxy. In 1988, the first example of an "Einstein ring" was discovered by Jackie Hewitt .