By the end of the next decade, we hope to have detected strongly lensed gravitational
waves by galaxies or clusters. Although there exist optimal methods for identifying lensed …

We apply a novel model based on convolutional neural networks (CNN) to identify
gravitationally lensed galaxies in multiband imaging of the Hyper Suprime-Cam Subaru …

More than 100 tidal disruption events (TDEs) have been detected at multiple bands, which
can be viewed as extreme laboratories to investigate the accretion physics and gravity in the …

Radio observations of strongly lensed objects are valuable as cosmological probes. Lensed
radio sources have proven difficult to identify, in large part due to the limited depth and …

Context. In the era of large-scale astronomical surveys, the fast modeling of strong lens
systems has become increasingly vital. While significant progress has been made for galaxy …

The mass distribution in massive elliptical galaxies encodes their evolutionary history, thus
providing an avenue to constrain the baryonic astrophysics in their evolution. The power-law …

We estimate the Einstein-radius-enclosed total mass for 177 cluster-scale strong
gravitational lenses identified by the ChicagO Optically selected Lenses Located At the …

The morphological diversity of galaxies is a relevant probe of galaxy evolution and
cosmological structure formation. However, in large sky surveys, even the morphological …

Context. With the current and upcoming generation of surveys, such as the Legacy Survey of
Space and Time (LSST) on the Vera C. Rubin Observatory and the Euclid mission, tens of …

The identification of strong gravitational lenses is essential to facilitate many studies in
astronomy. The search for strong gravitational lenses has become more challenging …