Spectroscopic Properties of the z = 4.5 Lyα --emitters

Astronomy and Astrophysics – Astronomy

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Scientific paper

We present Keck/LRIS and Keck/DEIMOS optical spectra of ˜ 50 star--forming galaxies at z ≈ 4.5 discovered in the Large Area Lyman Alpha (LALA) survey. The survey has identified a sample of ˜ 350 candidate Lyα --emitting galaxies at z ≈ 4.5 in a search volume of 1.5 × 106 comoving Mpc3; the spectroscopic confirmations presented herein suggest a selection reliability of ˜ 80%. The large equivalent widths (median Wλ rest} ≈ 80 Å) but narrow physical widths (Δ v < 500 km s-1) of the Lyα emission lines, along with the lack of accompanying high--ionization state emission lines, suggests that these galaxies are young systems powered by star formation rather than by AGN activity. Theoretical models of galaxy formation in the primordial Universe suggest that a small fraction of Lyα --emitting galaxies at z ≈ 4.5 may still be nascent, metal--free objects. Indeed, we find with 96% confidence that at least ˜ 20% of the confirmed sources show Wλ rest} > 240 Å, exceeding the maximum Lyα equivalent width predicted for normal stellar populations. Nonetheless, we find no evidence for \ion{He}{2} λ 1640 emission in either individual or composite spectra, indicating that though these galaxies are young, they are not truly primitive, Population III objects.

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