Connecting the escape fraction of Lyman-alpha and Lyman-continuum photons in star-forming galaxies at z 4-5
Abstract
We present a study of the connection between the escape fraction of Lyman-alpha (Lyα) and Lyman-continuum (LyC) photons within a sample of N=152 star-forming galaxies selected from the VANDELS survey at 3.85<zspec<4.95. By combining measurements of Hα equivalent width (Wλ(Hα)) derived from broad-band photometry with Lyα equivalent width (Wλ(Lyα)) measurements from VANDELS spectra, we individually estimate fescLyα for our full sample. In agreement with previous studies, we find a positive correlation between Wλ(Lyα) and fescLyα, increasing from fescLyα0.04 at Wλ(Lyα)=10A to fescLyα0.1 at Wλ(Lyα)=25A. For the first time at z4-5, we investigate the relationship between fescLyα and fescLyC using fescLyC estimates derived using the equivalent widths of low-ionization, FUV absorption lines in composite VANDELS spectra. Our results indicate that fescLyC rises monotonically with fescLyα, following the relation fescLyC 0.15+0.06-0.04fescLyα. Based on composite spectra of sub-samples with roughly constant Wλ(Lyα), but very different fescLyα, we show that the fescLyC-fescLyα correlation is not driven by a secondary correlation between fescLyαand Wλ(Lyα). The fescLyC-fescLyα correlation is in good qualitative agreement with theoretical predictions and provides further evidence that estimates of fescLyC within the Epoch of Reionization should be based on proxies sensitive to neutral gas density/geometry and dust attenuation.
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