We present a new model of the nebular emission from star-forming galaxies in a wide range
of chemical compositions, appropriate to interpret observations of galaxies at all cosmic …

ABSTRACT CLOUDY is a large‐scale spectral synthesis code designed to simulate fully
physical conditions within an astronomical plasma and then predict the emitted spectrum …

We make use of JWST medium-band and broadband NIRCam imaging, along with
ultradeep MIRI 5.6 μm imaging, in the Hubble eXtreme Deep Field to identify prominent line …

Starburst99 is a comprehensive set of model predictions for spectrophotometric and related
properties of galaxies with active star formation. The models are an improved and extended …

In this paper, we present high-resolution optical spectra and optical classifications from our
large sample of 285 warm infrared galaxies 10 8< L IR< 10 12.5 L☉. We have classified …

We present a new model for computing consistently the line and continuum emission from
galaxies, based on a combination of recent population synthesis and photoionization codes …

The reddening properties and the star formation history of a sample of 19 starburst galaxies
are investigated using multiwavelength spectroscopy and infrared broad band photometry …

We present the results of low-dispersion optical spectroscopy of 186 H II regions spanning a
range of radius in 13 spiral galaxies. Abundances for several elements (oxygen, nitrogen …

Following our study on the incidence, morphology and kinematics of the ionized gas in early-
type galaxies, we now address the question of what is powering the observed nebular …

Context. Identifying the physical mechanisms driving the escape of Lyman continuum (LyC)
photons is crucial for the search of Lyman continuum emitter (LCE) candidates. Aims. To …