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 …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

We present an overview of a new integral field spectroscopic survey called MaNGA
(Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the …

We present an overview of galaxy evolution across cosmic time in the Illustris simulation.
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …

ABSTRACT Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical
fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs …

The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …

In the cold dark matter cosmology, the baryonic components of galaxies—stars and gas—
are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter …

We present the clump populations detected in 18 lensed galaxies at redshifts 1--8.5 within
the lensing cluster field SMACS0723. The recent JWST Early Release Observations of this …

Using observations from the MOSFIRE Deep Evolution Field survey, we investigate the
physical conditions of star-forming regions in z∼ 2.3 galaxies, specifically the electron …

Abstract The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-
consistently understand the small-scale structure of the interstellar medium (ISM) and its link …