Context. The third Gaia data release (DR3) provides a wealth of new data products. The
early part of the release, Gaia EDR3, already provided the astrometric and photometric data …

We introduce an updated physical model to simulate the formation and evolution of galaxies
in cosmological, large-scale gravity+ magnetohydrodynamical simulations with the moving …

It is now 16 years since the first data release from the Sloan Digital Sky Survey (SDSS; York
et al. 2000). This Early Data Release, or EDR, occurred in 2001 June (Stoughton et al …

Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …

Abstract The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-
object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey …

Galaxy sizes and their evolution over cosmic time have been studied for decades and serve
as key tests of galaxy formation models. However, at z≳ 1 these studies have been limited …

We present the redshift evolution of the galaxy effective radius re obtained from the Hubble
Space Telescope (HST) samples of∼ 190,000 galaxies at z= 0–10. Our HST samples …

We analyse scaling relations and evolution histories of galaxy sizes in TNG100, part of the
IllustrisTNG simulation suite. Observational qualitative trends of size with stellar mass, star …

Abstract The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary
spectroscopic surveys of low redshift galaxies. Covering an area of∼ 286 deg2 (split among …

The tight correlations between the masses of supermassive black holes (BHs) and the
properties of their host galaxies suggest that BHs co-evolve with galaxies. However, what is …