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 …

Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm,[Oi] 63 μm,
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …

ABSTRACT A two-parameter semi-empirical model is presented for the spectral energy
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …

We report the results from a systematic search for molecular (OH 119 μm) outflows with
Herschel/PACS in a sample of 43 nearby (z< 0.3) galaxy mergers, mostly ultraluminous …

Mergers of galaxies are thought to cause significant gas inflows to the inner parsecs, which
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …

We present an atlas of 129 spectral energy distributions for nearby galaxies, with
wavelength coverage spanning from the ultraviolet to the mid-infrared. Our atlas spans a …

We present mid-infrared spectroscopic observations of the nucleus of the nearby Seyfert
galaxy NGC 7469 taken with the MIRI instrument on the James Webb Space Telescope …

We present the first results of a survey of the [C ii] 157.7 μm emission line in 241 luminous
infrared galaxies (LIRGs) comprising the Great Observatories All-sky LIRG Survey (GOALS) …

The merger of two or more galaxies can enhance the inflow of material from galactic scales
into the close environments of active galactic nuclei (AGNs), obscuring and feeding the …

ABSTRACT (Ultra) luminous infrared galaxies ((U) LIRGs) are objects characterized by their
extreme infrared (8–1000 μm) luminosities (L LIRG> 10 11 L☉ and L ULIRG> 10 12 L☉) …