By compiling a comprehensive census of literature studies, we investigate the evolution of
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …

We present the wide field slitless spectroscopy mode of the NIRISS instrument on the James
Webb Space Telescope. This mode employs two orthogonal low-resolution (resolving …

We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …

The nebular recombination line H α is widely used as a star formation rate (SFR) indicator in
the local and high-redshift Universe. We present a detailed H α radiative transfer study of …

We demonstrate that the inference of galaxy stellar masses via spectral energy distribution
(SED) fitting techniques for galaxies formed in the first billion years after the Big Bang carries …

At fixed galaxy stellar mass, there is a clear observational connection between structural
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …

We present predictions for the extent of the dust-continuum emission of main-sequence
galaxies drawn from the TNG50 simulation in the range z= 1–5. We couple the radiative …

With its exquisite sensitivity, wavelength coverage, and spatial and spectral resolution, the
James Webb Space Telescope (JWST) is poised to revolutionize our view of the distant …

Matching the number counts of high-z submillimetre-selected galaxies (SMGs) has been a
long-standing problem for galaxy formation models. In this paper, we use 3D dust radiative …

We use mock images of z= 0.1 galaxies in the 100 Mpc EAGLE simulation to establish the
differences between the sizes and morphologies inferred from the stellar mass distributions …