ABSTRACT I introduce some improvements to the ppxf method, which measures the stellar
and gas kinematics, star formation history (SFH) and chemical composition of galaxies. I …

Star-forming galaxies can in principle be transformed into passive systems by a multitude of
processes that quench star formation, such as the halting of gas accretion (starvation) or the …

We present the host galaxies of four apparently nonrepeating fast radio bursts (FRBs), FRB
20181223C, FRB 20190418A, FRB 20191220A, and FRB 20190425A, reported in the first …

The most direct and strongest evidence for the presence of dark energy is provided by the
measurement of galaxy distances using SNe Ia. This result is based on the assumption that …

Dynamical models are crucial for uncovering the internal dynamics of galaxies; however,
most of the results to date assume axisymmetry, which is not representative of a significant …

We perform full spectrum fitting stellar population analysis and Jeans Anisotropic modelling
of the stellar kinematics for about 2000 early-type galaxies (ETGs) and spiral galaxies from …

This is the second paper of the Map** Nearby Galaxies at Apache Point Observatory
(MaNGA) Dynamics and stellar Population (DynPop) series, which analyses the global …

We present the second major release of data from the Sydney–Australian Astronomical
Observatory Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey. Data Release …

Cosmological hydrodynamical simulations are rich tools to understand the build-up of stellar
mass and angular momentum in galaxies, but require some level of calibration to …

We analyze the stellar age indicators (D n 4000 and EW (Hδ)) and sizes of 467 quiescent
galaxies with M*≥ 10 10 M⊙ at z∼ 0.7 drawn from DR2 of the LEGA-C survey. Interpreting …