We introduce the first two simulations of the IllustrisTNG project, a next generation of
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …

We present emerge, an E mpirical M od E l for the fo R mation of G alaxi E s, describing the
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …

We present observations with the Cosmic Origins Spectrograph (COS) onboard the Hubble
Space Telescope of five star-forming galaxies at redshifts in the range 0.2993–0.4317 and …

We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …

The MOSDEF Survey: A Stellar Mass–SFR–Metallicity Relation Exists at z ∼ 2.3 - IOPscience
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The tight correlation between total galaxy stellar mass and star formation rate (SFR) has
become known as the star-forming main sequence. Using∼ 487 000 spaxels from galaxies …

The tidal disruption of a star by a massive black hole is expected to yield a luminous flare of
thermal emission. About two dozen of these stellar tidal disruption flares (TDFs) may have …

Major galaxy mergers are thought to play an important part in fuelling the growth of
supermassive black holes. However, observational support for this hypothesis is mixed, with …

We study radial profiles in H α equivalent width and specific star formation rate (sSFR)
derived from spatially resolved SDSS-IV MaNGA spectroscopy to gain insight on the …

The SHINING survey offers a great opportunity to study the properties of the ionized and
neutral media of galaxies from prototypical starbursts and active galactic nuclei (AGNs) to …