I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

Supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …

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 a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk
Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …

In this paper we study a key phase in the formation of massive galaxies: the transition of star-
forming galaxies into massive (M stars∼ 10 11 M⊙), compact (re∼ 1 kpc) quiescent …

We study the growth of massive galaxies from z= 2 to the present using data from the
NOAO/Yale NEWFIRM Medium Band Survey. The sample is selected at a constant number …

Using cosmological simulations, we address the interplay between structure and star
formation in high-redshift galaxies via the evolution of surface density profiles. Our sample …

We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01<
z< 0.1 (8399 galaxies in g to K s bands) to derive the stellar mass–half-light radius relations …

Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and
Quiescent Galaxies - IOPscience This site uses cookies. By continuing to use this site you …