The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

The relation between galaxy stellar mass and gas-phase metallicity is a sensitive diagnostic
of the main processes that drive galaxy evolution, namely cosmological gas inflow, metal …

Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …

We derive new empirical calibrations for strong-line diagnostics of gas phase metallicity in
local star forming galaxies by uniformly applying the Te method over the full metallicity range …

We use a sample of 87 rest-frame UV-selected star-forming galaxies with mean
spectroscopic redshift⟨ z⟩= 2.26±0.17 to study the correlation between metallicity and …

We present intermediate-resolution optical spectrophotometry of 65 galaxies obtained in
support of the Spitzer Infrared Nearby Galaxies Survey (SINGS). For each galaxy we obtain …

We have investigated the mass-metallicity (MZ) relation using galaxies at 0.4< z< 1.0 from
the Gemini Deep Deep Survey (GDDS) and Canada-France Redshift Survey (CFRS). Deep …

Generally the gas metallicity in distant galaxies can only be inferred by using a few
prominent emission lines. Various theoretical models have been used to predict the …

We study the relation between nitrogen and oxygen abundances as a function of metallicity
for a sample of emission-line objects for which a direct measurement of the metallicity has …

ABSTRACT The CHemical Abundances of Spirals (CHAOS) project leverages the combined
power of the Large Binocular Telescope (LBT) with the broad spectral range and sensitivity …