Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

We present a comprehensive analysis of the evolution of the morphological and structural
properties of a large sample of galaxies at z= 3–9 using early James Webb Space …

We present reduced data and data products from the 3D-HST survey, a 248-orbit HST
Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five …

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

We present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering
90% of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h …

The interplay between cosmic gas accretion on to galaxies and galaxy mergers drives the
observed morphological diversity of galaxies. By comparing the state-of-the-art …

We report two secure (= z 3.775, 4.012) and one tentative (z≈ 3.767) spectroscopic
confirmations of massive and quiescent galaxies through K-band observations with …

We use the Illustris simulation to study the relative contributions of in situ star formation and
stellar accretion to the build-up of galaxies over an unprecedentedly wide range of masses …

We use cosmological simulations to study a characteristic evolution pattern of high-redshift
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …