A likelihood-based method for measuring weak gravitational lensing shear in deep galaxy
surveys is described and applied to the Canada–France–Hawaii Telescope (CFHT) Lensing …

We point out a natural mechanism for quenching of star formation in early-type galaxies
(ETGs). It automatically links the color of a galaxy with its morphology and does not require …

We describe and test the pipeline used to measure the weak-lensing shear signal from the
Kilo-Degree Survey (KiDS). It includes a novel method of 'self-calibration'that partially …

A century ago, in 1911 and 1913, Plummer and then Reynolds introduced their models to
describe the radial distribution of stars innebulae'. This article reviews the progress since …

We describe and discuss the selection procedure and statistical properties of the galaxy
sample used by the Calar Alto Legacy Integral Field Area (CALIFA) survey, a public legacy …

We present a self-consistent model of the spectral energy distributions (SEDs) of spiral
galaxies from the ultraviolet (UV) to the mid-infrared (MIR)/far-infrared (FIR)/submillimeter …

We present the results of two-component (disc+ bar) and three-component (disc+ bar+
bulge) multiwavelength 2D photometric decompositions of barred galaxies in five Sloan …

Fast radio bursts (FRBs) are a newly discovered class of extragalactic radio transients
characterized by their high energy and short duration (from microseconds to milliseconds) …

We investigate the effect of dust on spiral galaxies by measuring the inclination dependence
of optical colours for 24 276 well-resolved Sloan Digital Sky Survey (SDSS) galaxies visually …

Gradients in the mass-to-light ratio of distant galaxies impede our ability to characterize their
size and compactness. The long-wavelength filters of JWST's NIRCam offer a significant …