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< …

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 apply the radiative transfer (RT) code skirt on a sample of low-redshift (z≤ 0.1) galaxies
extracted from the TNG50 simulation to enable an apples-to-apples comparison with …

We present powderday (available at https://github. com/dnarayanan/powderday), a flexible,
fast, open-source dust radiative transfer package designed to interface with both idealized …

We present a framework to build realistic mock spectroscopic observations for state-of-the-
art hydrodynamical simulations, using high spectral resolution stellar population models and …

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 …

We present the eddington bias corrected specific star formation rate function (sSFRF) at
different stellar mass scales from a sub-sample of the Sloan Digital Sky Survey Data …

Aims. Current hydrodynamical and semi-empirical simulations of galaxy formation and
evolution have difficulties in reproducing the number densities of infrared-detected galaxies …

We present a comparative study of four physical dust models and two single-temperature
modified blackbody models by fitting them to the resolved WISE, Spitzer, and Herschel …

A debate is emerging regarding the recent inconsistent results of different studies for the
cosmic star formation rate density (CSFRD) at high-z. We employ UV and IR data sets to …