We present a large set of theoretical isochrones, whose distinctive features mostly reside on
the greatly-improved treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) …

We present predictions for the evolution of the galaxy dust-to-gas ratio (DGR) and dust-to-
metal ratio (DTM) from z= 0→ 6, using a model for the production, growth, and destruction of …

We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …

We make use of Atacama Large Millimeter/submillimeter Array continuum observations of 15
luminous Lyman-break galaxies at z∼ 7–8 to probe their dust-obscured star formation …

Context. The efficiency of the different processes responsible for the evolution of interstellar
dust on the scale of a galaxy are, to date, very uncertain, spanning several orders of …

We report far-infrared and submillimeter observations of supernova 1987A, the star whose
explosion was observed on 23 February 1987 in the Large Magellanic Cloud, a galaxy …

We present IRAM/NOEMA and JVLA observations of the quasar J1342+ 0928 at z= 7.54 and
report detections of copious amounts of dust and [C ii] emission in the interstellar medium …

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 …

Aims. We studied the evolution of the abundance in interstellar dust species that originate in
stellar sources and from condensation in molecular clouds in the local interstellar medium of …

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 …