Strong Gravitational Lensing with the James Webb Space Telescope
Adi Zitrin

TL;DR
This paper discusses how the James Webb Space Telescope enhances the study of strong gravitational lensing, enabling unprecedented observations of distant cosmic sources and dark matter distribution.
Contribution
It summarizes recent advances and future prospects of strong gravitational lensing research utilizing JWST's capabilities.
Findings
Enhanced detection of distant sources due to JWST's sensitivity.
Improved understanding of dark matter through lensing observations.
Potential for new discoveries in high-resolution astrophysics.
Abstract
The theory of General Relativity predicts that, since massive bodies curve spacetime, light from a distant source would be deflected by a foreground massive object -- a phenomenon known as \emph{Gravitational Lensing}. Historically, the strength of deflection of light from background stars by the sun, during the 1919 solar eclipse, supplied one of the first proofs for the theory of General Relativity. However, it is only in the last few decades, with the advent of the Hubble Space Telescope and other large, ground-based facilities, that lensing has become a principal tool in modern astronomy. Lensing allows us to study both the matter content of the lensing bodies such as galaxies or clusters of galaxies, mainly dominated by the otherwise-invisible \emph{dark matter}, and the distant background sources that are being lensed by them. Strong gravitational lensing, where sources are…
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