Context. Strongly star-forming galaxies of subsolar metallicities are typical of the high-
redshift universe. Here we therefore provide accurate data for two low-z analogs, the well …

Context. The low-metallicity interstellar medium (ISM) is profoundly different from that of
normal systems, being clumpy with low dust abundance and little CO-traced molecular gas …

We present far infrared (FIR) spectroscopy of the luminous blue compact galaxy (BCG) Haro
11 (ESO 350-IG38) obtained with the ISO Long Wavelength Spectrometer (LWS) in low …

Ultra-strong emission-line galaxies (USELs) with extremely high equivalent widths (EW
(Hβ)≳ 30 Å) can be used to pick out galaxies of extremely low metallicity in the z= 0–1 …

Context. Intermediate mass galaxies (> 10 10) at z~ 0.6 are the likeliest progenitors of the
present-day, numerous population of spirals. There is growing evidence that they have …

Recently, Kojima and co-authors have reported a record low oxygen abundance, 12+
logO/H= 6.90±0.03, or 1.6 per cent of solar metallicity, in the low-mass star-forming galaxy …

We present a sample of four emission-line galaxies at z= 6.11–6.35 that were
serendipitously discovered using the commissioning data for the James Webb Space …

We present the results of near-infrared spectroscopic observations for a sample of 12 star-
forming galaxies at 1.0< z< 1.5, drawn from the DEEP2 Galaxy Redshift Survey. Hβ,[O III] …

The C iii] 1909 (hereafter C iii]) line is the strongest ultraviolet emission line after Lyα and is
therefore of interest to high-redshift studies of star-forming (SF) galaxies near the epoch of …

ABSTRACT We present VLT/X-Shooter and MUSE spectroscopy of a faint F814W=
28.60±0.33 (${M} _ {\mathrm {UV}}=-17.0$), low-mass (≲ ${10}^{7}{M} _ {\odot} $), and …