We investigate the star-forming main sequence of the host galaxies of a large, well-defined
sample of 453 redshift∼ 0.3 quasars with previously available star formation rates by …

Despite the importance of feedback from active galactic nuclei (AGNs) in models of galaxy
evolution, observational constraints on the influence of AGN feedback on star formation …

Central molecular outflows in spiral galaxies are assumed to modulate their host galaxy's
star formation rate (SFR) by removing gas from the inner region of the galaxy. Outflows …

We present an improved study of the relation between supermassive black hole growth and
their host galaxy properties in the local Universe (z< 0.33). To this end, we build an …

We present high-resolution (∼ 2.4 kpc) ALMA band 7 observations (rest-frame λ∼ 250 m) of
three powerful z∼ 2.5 quasars (L bol= 1047.3–1047.5 erg s− 1). These targets have …

The missing mass problem has been with us since the 1970s, as Newtonian gravity using
baryonic mass cannot account for various observations. We investigate the viability of …

Context. Large-scale cosmological simulations suggest that feedback from active galactic
nuclei (AGN) plays a crucial role in galaxy evolution. More specifically, outflows are one of …

We present spatially resolved gas kinematics, ionization, and energetics of 11 type 1 and 5
type 2 active galactic nuclei (AGNs) with strong ionized gas outflows at z< 0.3 using Gemini …

We present rest-frame ultraviolet images of six luminous quasars at z∼ 4.8 obtained with the
Hubble Space Telescope (HST). These quasars exhibit a wide range of star formation rates …

There is an ongoing debate on whether feedback from active galactic nuclei (AGNs) can
effectively regulate the star formation activities in their host galaxies. To investigate the …