arXiv · 1201.5630
Stacked Rest-Frame UV Spectra of Ly$α$-Emitting and Continuum-Selected Galaxies at 2<z<3.5
Abstract
We present properties of individual and composite rest-UV spectra of continuum- and narrowband-selected star-forming galaxies (SFGs) at a redshift of 2 20 Å, the canonical limit to be classified as a LAE. We divide our dataset into subsamples based on properties we are able to measure for each individual galaxy: Lyα equivalent width, rest-frame UV colors, and redshift. Among our subsample of galaxies with R<25.5, those with rest-frame W_{Lyα}>20 Å have bluer UV continua, weaker low-ionization interstellar absorption lines, weaker C IV absorption, and stronger Si II* nebular emission than those with W_{Lyα}<20 Å. We measure a typical velocity offset of Δv~600 km s$^{-1}$ between Lyα emission and low-ionization absorption among our subsamples. We find that the interstellar component, as opposed to the stellar component, dominates the high-ionization absorption line profiles. We find the low- and high-ionization Si ionization states have similar kinematic properties, yet the low-ionization absorption is correlated with Ly$α$ emission and the high-ionization absorption is not. These trends are consistent with outflowing neutral gas being in the form of neutral clouds embedded in ionized gas as previously suggested by \cite{Steidel2010}. Moreover, our galaxies with bluer UV colors have stronger Lyα emission, weaker low-ionization absorption and more prominent nebular emission line profiles. Among our dataset, UV-bright galaxies with W_{Lyα}>20 Å exhibit weaker Lyα emission at lower redshifts, although we caution that this could be caused by spectroscopic confirmation of low Lyα equivalent width galaxies being harder at z~3 than z~2.
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Michael Berry, Eric Gawiser, Lucia Guaita, Nelson Padilla, Ezequiel Treister, Guillermo Blanc, Robin Ciardullo, Harold Francke, Caryl Gronwall. 2012-01-26. Stacked Rest-Frame UV Spectra of Ly$α$-Emitting and Continuum-Selected Galaxies at 2<z<3.5. https://doi.org/10.1088/0004-637x%2F749%2F1%2F4
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