Page 2: Research news on Gravitational lensing

Gravitational lensing as a research area investigates the deflection, magnification, and distortion of light from distant sources by intervening mass distributions, as predicted by general relativity, and develops methods to use these effects as astrophysical and cosmological probes. It encompasses strong, weak, and microlensing regimes, focusing on reconstructing mass profiles of galaxies and clusters, mapping dark matter, constraining dark energy via lensing statistics and cosmic shear, and testing gravity on large scales. The field integrates theoretical modeling, numerical simulations, and analysis of large imaging and spectroscopic surveys, emphasizing inverse problems, bias control, and statistical inference to extract cosmological parameters and substructure properties.

Using bent light to map complex planetary architectures

With new technologies comes new discoveries. Or so Spider Man's Uncle Ben might have said if he was an astronomer. Or a scientist more generally—but in astronomy that saying is more true than many other disciplines, as ...

Machine learning discovers quasars acting as lenses

Quasars acting as strong gravitational lenses are among the rarest finds in astronomy. Out of nearly 300,000 quasars cataloged in the Sloan Digital Sky Survey, only twelve candidates were identified, and just three confirmed. ...

Gravitational lenses imaged by Webb during its first run

Periodically, the European Space Agency (ESA) releases images that provide breathtaking views of the cosmos, courtesy of its premier missions. This includes a relative newcomer to party with the ESA/Webb Picture of the Month, ...

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