activity
20182022
most citedMETAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity

55 citations · 80 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.IM20221 cited

The CUBES Science Case

Chris Evans, Stefano Cristiani, Cyrielle Opitom +51

We introduce the scientific motivations for the development of the Cassegrain U-Band Efficient Spectrograph (CUBES) that is now in construction for the Very Large Telescope. The as…

astro-ph.GA202255 cited

METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity

J. Roman-Duval, E. B. Jenkins, K. Tchernyshyov +9

The metallicity and gas density dependence of interstellar depletions, the dust-to-gas (D/G), and dust-to-metal (D/M) ratios have important implications for how accurately we can t…

astro-ph.GA20217 cited

H_2 molecular gas absorption-selected systems trace CO molecular gas-rich galaxy overdensities

Anne Klitsch, Celine Peroux, Martin A. Zwaan +3

Absorption-selected galaxies offer an effective way to study low-mass galaxies at high redshift. However, the physical properties of the underlying galaxy population remains uncert…

astro-ph.IM2021

Exploration of the high-redshift universe enabled by THESEUS

N. R. Tanvir, E. Le Floc'h, L. Christensen +36

At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star f…

astro-ph.GA201917 cited

Dust-depletion sequences in damped Ly-α absorbers II. The composition of cosmic dust, from low-metallicity systems to the Galaxy

Lars Mattsson, Annalisa De Cia, Anja C. Andersen +1

We aim at assessing what are the most dominant dust species or types, including silicate and iron oxide grains present in the ISM, by using recent observations of dust depletion of…

astro-ph.HE2018

A UV Resonance Line Echo from a Shell Around a Hydrogen-Poor Superluminous Supernova

R. Lunnan, C. Fransson, P. M. Vreeswijk +21

Hydrogen-poor superluminous supernovae (SLSN-I) are a class of rare and energetic explosions discovered in untargeted transient surveys in the past decade. The progenitor stars and…