This paper presents a study of the local radio source population, by cross-comparing the
data from the first data release (DR1) of the LOFAR Two-Metre Sky Survey (LoTSS) with the …

We constructed a sample of 23 344 radio-loud active galactic nuclei (RLAGN) from the
catalogue derived from the LOFAR Two-Metre Sky Survey (LoTSS) survey of the HETDEX …

The traditional picture of post-starburst galaxies as dust-and gas-poor merger remnants,
rapidly transitioning to quiescence, has been recently challenged. Unexpected detections of …

The goal of population spectral synthesis (pss; also referred to as inverse, semi-empirical
evolutionary-or fossil record approach) is to decipher from the spectrum of a galaxy the …

It is well established that active galactic nuclei (AGNs) play an important role in the evolution
of galaxies. These AGNs can be linked to the accretion processes onto massive black holes …

The effects of feedback from high luminosity radio-loud active galactic nuclei (AGN) have
been extensively discussed in the literature, but feedback from low-luminosity radio-loud …

We study the population of active galaxies in void environment in the Sloan Digital Sky
Survey. We use optical spectroscopic information to analyse characteristics of the emission …

Combining the cloudy photoionization code with updated stellar population synthesis
results, we simultaneously model the MIR versus, the MIR-FIR versus and the classical BPT …

Supernovae (SNe) inject∼ 1051 erg in the interstellar medium, thereby shocking and
heating the gas. A substantial fraction of this energy is later lost via radiative cooling. We …

The effect of active galactic nuclei (AGN) on their host galaxies–in particular their levels of
star formation–remains one of the key outstanding questions of galaxy evolution. Successful …