Results 101 to 110 of about 70,851 (245)
Effects of Disks on Gravitational Lensing by Spiral Galaxies [PDF]
Matthias Bartelmann +3 more
openalex +1 more source
Algebraic Properties of the Real Quintic Equation for a Binary Gravitational Lens [PDF]
Hideki Asada, T. Kasai, M. Kasai
openalex +1 more source
The Evolution of Gravitational Lens Galaxies
Most gravitational lens galaxies are early-type galaxies in relatively low density environments. We show that they lie on the same fundamental plane as early-type galaxies in both local and distant rich clusters. Their surface brightness evolution requires a typical star formation epoch of z=2-3, almost indistinguishable from that of rich cluster ...
Kochanek, C. S. +8 more
openaire +2 more sources
Brane world cosmologies and statistical properties of gravitational lenses [PDF]
Deepak Jain, A. Dev, J. S. Alcaniz
openalex +1 more source
Lensing Point-spread Function of Coherent Astrophysical Sources and Nontrivial Wave Effects
Most research on astrophysical lensing has been conducted using the geometric optics framework, where there exists a clear concept of lensing images. However, wave optics effects can be important for coherent sources, e.g., pulsars, fast radio bursts ...
Xun Shi
doaj +1 more source
Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). I. Automatic search for galaxy-scale strong lenses [PDF]
Alessandro Sonnenfeld +14 more
openalex +1 more source
Observed evolution of the total mass distribution with redshift is crucial to testing galaxy evolution theories. To measure the total mass distribution, strong gravitational lenses complement the resolved dynamical observations that are currently limited
Nandini Sahu +15 more
doaj +1 more source
Gravitational lensing detection of an extremely dense environment around a galaxy cluster [PDF]
M. Sereno +10 more
openalex +1 more source
First Resolution of Microlensed Images of a Binary-lens Event
We resolve the multiple images of the binary-lens microlensing event ASASSN-22av using the GRAVITY instrument of the Very Large Telescope Interferometer (VLTI).
Zexuan Wu +75 more
doaj +1 more source

