The emission line properties of gravitationally lensed 1.5<z<5 galaxies

Abstract

We present and analyse near-infrared spectroscopy for a sample of 28 gravitationally lensed star-forming galaxies in the redshift range 1.5 < z < 5, observed mostly with the Keck II telescope. With typical magnifications of ≃1.5–4 mag, our survey provides a valuable census of star formation rates, gas-phase metallicities and dynamical masses for a representative sample of low-luminosity galaxies seen at a formative period in cosmic history. We find less evolution in the mass–metallicity relation compared to earlier work that focused on more luminous systems with z ~ 2–3, especially in the low mass (~10^9 M_⊙) where our sample is ~0.25 dex more metal-rich. We interpret this offset as a result of the lower star formation rates (typically a factor of ~10 lower) for a given stellar mass in our subluminous systems. Taking this effect into account, we conclude our objects are consistent with a fundamental metallicity relation recently proposed from unlensed observations.

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