We present photoionization modeling of galaxy populations at z∼ 0, 2, and> 6 to bridge
optical and far-infrared (FIR) emission-line diagrams. We collect galaxies with …

Context. Future and ongoing infrared and radio observatories such as JWST, METIS, and
ALMA will increase the amount of rest-frame IR spectroscopic data for galaxies by several …

We present an overview of the high-redshift extragalactic science case for the Single
Aperture Large Telescope for Universe Studies (SALTUS) far-infrared (IR) National …

We present updated measurements of the [O iii] 88 μm,[C ii] 158 μm, and dust continuum
emission from a star-forming galaxy at z= 7.212, SXDF-NB1006-2, by utilizing Atacama …

Mass loss is one of the key parameters that determine stellar evolution. Despite the progress
we have achieved over the last decades we still cannot match the observational derived …

Context. Massive star formation leads to enrichment of the interstellar medium with heavy
elements. On the other hand, the abundance of heavy elements is a key parameter with …

Context. The infrared (IR) range is extremely useful in the context of chemical abundance
studies of the gas-phase interstellar medium (ISM) due to the large variety of ionic species …

Context. Episodic mass-loss events such as giant eruptions in luminous blue variables or
pre-supernova eruptions in red supergiants drastically alter the evolutionary path of a …

Polycyclic aromatic hydrocarbon (PAH) dust emission has been proposed as an effective
extinction-independent star formation rate (SFR) indicator in the mid-infrared, but this may …

We present the [O III] λ52 μm map of the dwarf galaxy IC 10 obtained with the Field-Imaging
Far-Infrared Line Spectrometer on board the Stratospheric Observatory for Infrared …