Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …

We present the scientific program of the Spectr-M project aimed at the creation and
operation of the Millimetron Space Observatory (MSO) planned for launch in the late 2020s …

According to the current understanding of cosmic structure formation, the precursors of the
most massive structures in the Universe began to form shortly after the Big Bang, in regions …

The estimated stellar masses of galaxies are widely used to characterize how the galaxy
population evolves over cosmic time. If stellar masses can be estimated in a robust manner …

We present Herschel observations of 6 fine-structure lines in 25 ultraluminous infrared
galaxies at z< 0.27. The lines,[O iii] 52 μm,[N iii] 57 μm,[O i] 63 μm,[N ii] 122 μm,[O i] 145 μm …

We have fit the far-ultraviolet (FUV) to sub-millimeter (850 μm) spectral energy distributions
(SEDs) of the 61 galaxies from the Key Insights on Nearby Galaxies: A Far-Infrared Survey …

We present full-volume cosmological simulations, using the moving-mesh code arepo to
study the coevolution of dust and galaxies. We extend the dust model in arepo to include …

The total infrared (IR) luminosity is very useful for estimating the star formation rate (SFR) of
galaxies, but converting the IR luminosity into an SFR relies on assumptions that do not hold …

In this work, we investigate the far-ultraviolet (UV) to near-infrared (NIR) shape of the dust
attenuation curve of a sample of IR-selected dust obscured (ultra) luminous IR galaxies at …

Context. In recent observations of extremely metal-poor, low-mass, starburst galaxies,
almost solar Fe/O ratios are reported, despite N/O ratios consistent with the low metallicity …