Ultralight Dark Matter Resonates with Binary Pulsars

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The microlensing signal in the light curves of gravitationally lensed quasars can shed light on the dark matter (DM) composition in their lensing galaxies. Here, we investigate a sample of six lensed quasars from the most recent and best COSMOGRAIL observa ...

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Galaxy-scale gravitational lenses are often modeled with two-component mass profiles where one component represents the stellar mass and the second is a Navarro Frenk White (NFW) profile representing the dark matter. Outside of the spherical case, the NFW ...

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Ultralight Dark Matter Resonates with Binary Pulsars

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The formation of the faintest galaxies in cosmological simulations: from the impact of primordial magnetic fields to the metal enrichment of present day dwarfs by first stars

Gaia Focused Product Release: Asteroid orbital solution: Properties and assessment

The impact of human expert visual inspection on the discovery of strong gravitational lenses

Probing the faint-end luminosity function of Lyman-alpha emitters at 3 < z < 7 behind 17 MUSE lensing clusters

Probing compact dark matter objects with microlensing in gravitationally lensed quasars

Probing the nature of Dark Energy through the study of large scale structures using spectroscopic surveys and their simulations

Dilute neutron star matter from neural-network quantum states

Potential scientific synergies in weak lensing studies between the CSST and Euclid space probes

Gravitationally lensed quasars in Gaia - IV. 150 new lenses, quasar pairs, and projected quasars

The ellipticity parameterization for an NFW profile: An overlooked angular structure in strong lens modeling

Liquid film instability of an internally coated horizontal tube