Determining the atomic and molecular content of the interstellar medium (ISM) is of
fundamental importance to understand the star-formation process. Although there exist …

Intracluster light (ICL) provides an important record of the interactions galaxy clusters have
undergone. However, we are limited in our understanding by our measurement methods. To …

Submillimeter emission lines produced by the interstellar medium (ISM) are strong tracers of
star formation and are some of the main targets of line intensity mapping (LIM) surveys. In …

Using a suite of 3D hydrodynamical simulations of star-forming molecular clouds, we
investigate how the density probability distribution function (PDF) changes when including …

Extended [CII] emission on tens of kiloparsecs, also known as a [CII] halo, is currently being
reported around z∼ 4− 6 star-forming galaxies, especially thanks to the statistics of the …

We present slick (the Scalable Line Intensity Computation Kit), a software package that
calculates realistic CO,[C i], and [C ii] luminosities for clouds and galaxies formed in …

Line-intensity mapping (LIM) is a promising technique to constrain the global distribution of
galaxy properties. To combine LIM experiments probing different tracers with traditional …

Galaxy morphology is a powerful diagnostic to assess the realism of cosmological
hydrodynamical simulations. Determining the morphology of simulated galaxies requires the …

In recent years, it has been speculated that in extreme low-metallicity galactic environments,
stars form in regions that lack H2. In this paper, we investigate how changing the metallicity …

The chemical enrichment of dust and metals are vital processes in constraining the star
formation history of the universe. These are important ingredients in the formation and …