We evaluate the redshift distribution of binary black hole (BBH), black hole–neutron star
binary (BHNS), and binary neutron star (BNS) mergers, exploring the main sources of …

We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …

We present the photometric properties of galaxies in the First Light And Reionization Epoch
Simulations (FLARES). The simulations trace the evolution of galaxies in a range of …

ABSTRACT We introduce the First Light And Reionisation Epoch Simulations (FLARES), a
suite of zoom simulations using the EAGLE model. We resimulate a range of overdensities …

ABSTRACT The long anticipated James Webb Space Telescope (JWST) will be able to
directly detect large samples of galaxies at very high redshift. Using the well-established …

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 …

ABSTRACT The Nancy Grace Roman Space Telescope, NASA's next flagship observatory,
will redefine deep-field galaxy survey with a field of view two orders of magnitude larger than …

The detection rate of electromagnetic (EM) and gravitational wave (GW) transients is
growing exponentially. As the accuracy of the transient rates will significantly improve over …

Observations have revealed that the star formation rate (SFR) and stellar mass (M star) of
star-forming galaxies follow a tight relation known as the galaxy main sequence. However …

We use two independent galaxy-formation simulations, flares, a cosmological
hydrodynamical simulation, and shark, a semi-analytic model, to explore how well the JWST …