Sufficiently compact astrophysical objects can produce mirror-like reflection images of sources through extreme gravitational lensing in Schwarzschild spacetime.
Mea- suring the black hole and accretion parameters of sagit- tarius a* from eht observations using a semi-analytic model
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Revisiting The Gravitational Mirroring In Presence of Compact Objects
Sufficiently compact astrophysical objects can produce mirror-like reflection images of sources through extreme gravitational lensing in Schwarzschild spacetime.