The universe's biggest galaxies have both vast atmospheres and supermassive central
black holes. This article reviews how those two components of a large galaxy couple and …

Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

We present rest-frame optical data of the compact z= 5.55 galaxy GS_3073 obtained using
the integral field spectroscopy mode of the Near-InfraRed Spectrograph on board the James …

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 …

Understanding the variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …

We report on the host properties of five X-ray-luminous active galactic nuclei (AGN)
identified at 3< z< 5 in the first epoch of imaging from the Cosmic Evolution Early Release …

JWST has detected many overmassive galactic systems at z> 4, where the mass of the black
hole, M•, is 10–100 times larger than expected from local relations, given the host's stellar …

We reliably extend the stellar mass–size relation over 0.2≤ z≤ 2 to low stellar mass
galaxies by combining the depth of Hubble Frontier Fields with the large volume covered by …

Feedback from accreting supermassive black holes (SMBHs) is thought to be a primary
driver of quenching in massive galaxies, but how to best implement SMBH physics into …