This paper presents new deep and wide narrow-band surveys undertaken with United
Kingdom Infrared Telescope (UKIRT), Subaru and the Very Large Telescope (VLT), a …

We present a multi-epoch analysis of the galaxy populations formed within the cosmological
hydrodynamical simulations presented in Vogelsberger et al. These simulations explore the …

We present the first results from a near-IR spectroscopic survey of the COSMOS field, using
the Fiber Multi-Object Spectrograph on the Subaru telescope, designed to characterize the …

We present results from near-infrared spectroscopy of 26 emission-line galaxies at z∼ 2.2
and z∼ 1.5 obtained with the Folded-port InfraRed Echellette (FIRE) spectrometer on the 6.5 …

The nature of dust in distant galaxies is not well understood, and until recently few direct
dust measurements have been possible. We investigate dust in distant star-forming galaxies …

We present the first direct and unbiased measurement of the evolution of the dust mass
function of galaxies over the past 5 billion years of cosmic history using data from the …

We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of
galaxy populations at redshifts from z≈ 0 to= 8 in a full cosmological framework. We achieve …

We explore a large uniformly selected sample of Hα selected star-forming galaxies (SFGs) at
z= 0.40, 0.84, 1.47, 2.23 to unveil the evolution of the star formation rate (SFR) function and …

We use a semi-analytic model for disk galaxies to explore the origin of the time evolution
and small scatter of the galaxy SFR sequence–the tight correlation between star formation …

The nature of galaxies selected at submillimeter wavelengths (SMGs, S 850≳ 3 mJy), some
of the bolometrically most luminous objects at high redshifts, is still elusive. In particular their …