Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

▪ Abstract Meteorites and interplanetary dust particles contain presolar stardust grains: solid
samples of stars that can be studied in the laboratory. The stellar origin of the grains is …

We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

Abstract We present the Atacama Large Millimeter/submillimeter Array detection of the [O iii]
88 μm line and rest-frame 90 μm dust continuum emission in a Y-dropout Lyman break …

High-power lasers that fit into a university-scale laboratory can now reach focused
intensities of more than 1019 W cm-2 at high repetition rates. Such lasers are capable of …

Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …

Spectral energy distribution (SED) fitting in the far-infrared (FIR) is greatly limited by a dearth
of data and an excess of free parameters–from galaxies' dust composition, temperature …

Infrared spectroscopy provides a direct handle on the composition and structure of
interstellar dust. We have studied the dust along the line of sight toward the Galactic center …

Dust grains play a crucial role in the formation and evolution history of stars and galaxies in
the early universe. We investigate the formation of dust grains in the ejecta of Population III …

The presence of dust at high redshift requires efficient condensation of grains in supernova
(SN) ejecta, in accordance with current theoretical models. Yet observations of the few well …