We present deep ALMA dust continuum observations for a sample of luminous (M UV<− 22)
star-forming galaxies at z≃ 7. We detect five of the six sources in the far-infrared (FIR) …

Structural Evolution in Massive Galaxies at z ∼ 2 - IOPscience This site uses cookies. By
continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and …

We utilised the unprecedented depth and resolution of recent early-release science (ERS)
JWST observations to define the near-infrared counterparts of sub-millimetre galaxies …

We report morphological analyses of seven submillimeter galaxies (SMGs) at z∼ 2 using
the James Webb Space Telescope NIRCam images taken as part of the public CEERS and …

Large-scale outflows are believed to be an important mechanism in the evolution of
galaxies. We can determine the impact of these outflows by studying either current galaxy …

Aims. We aim to constrain for the first time the mean mass and extent of the molecular gas of
a mass-complete sample of normal> 10 10 M⊙ star-forming galaxies at 0.4< z< 3.6 …

Recent years have seen growing interest in post-processing cosmological simulations with
radiative transfer codes to predict observable fluxes for simulated galaxies. However, this …

We study the morphological properties of mid-infrared selected galaxies at 1.0< z< 1.7 in the
SMACS J0723. 3-7327 cluster field to investigate the mechanisms of galaxy mass assembly …

Aims. We study the stellar (ie, rest-optical) and dust-obscured star-forming (ie, rest-mid-
infrared) morphologies (ie, sizes and Sérsic indices) of star-forming galaxies (SFGs) at 0.1< …

We present high-resolution (∼ 2.4 kpc) ALMA band 7 observations (rest-frame λ∼ 250 m) of
three powerful z∼ 2.5 quasars (L bol= 1047.3–1047.5 erg s− 1). These targets have …