We present the first results from the Mapping Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …

Star formation rate (SFR) measurements at z> 4 have relied mostly on the rest-frame far-
ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-β …

We present the first observational infrared luminosity function (IRLF) measurement in the
Epoch of Reionization (EoR) based on a ultraviolet (UV)-selected galaxy sample with the …

We apply the spectral energy distribution (SED) fitting code ProSpect to multiwavelength
imaging for∼ 7000 galaxies from the GAMA survey at z< 0.06, in order to extract their star …

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 …

The intensity mapping of the [CII] 158-μm line redshifted to the submillimeter window is a
promising probe of the z> 4 star formation and its spatial distribution into large-scale …

We combine the shark semi-analytic model of galaxy formation with the prospect software
tool for spectral energy distribution (SED) generation to study the multiwavelength emission …

Simulations predict that the galaxy populations inhabiting protoclusters may contribute
considerably to the total amount of stellar mass growth of galaxies in the early universe. In …

ABSTRACT Using the First Light And Reionisation Epoch Simulations (flares), we explore
the dust-driven properties of massive high-redshift galaxies at z∈[5, 10]. By post-processing …

Submillimetre galaxies (SMGs) have long posed a challenge for theorists, and self-
consistently reproducing the properties of the SMG population in a large-volume …