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The Lyman Continuum Escape Fraction of Low-Mass Star-Forming Galaxies at z~1

, , , , , , , , , , , , and .
(2015)cite arxiv:1511.01998Comment: submitted for second review to ApJ.

Abstract

To date no direct detection of Lyman continuum emission has been measured for intermediate--redshift z~1 star-forming galaxies . We combine HST grism spectroscopy with GALEX UV and ground--based optical imaging to extend the search for escaping Lyman continuum to a large (~600) sample of z~1 low-mass, moderately star-forming galaxies selected initially on H$\alpha$ emission. The characteristic escape fraction of LyC from SFGs that populate this parameter space remains weakly constrained by previous surveys, but these faint SFGs are assumed to play a significant role in the reionization of neutral hydrogen in the intergalactic medium (IGM) at high redshift (z>6). We do not make an unambiguous detection of escaping LyC radiation from this $z\sim1$ sample, individual non--detections to constrain the absolute Lyman continuum escape fraction, $f_esc$<2.1% (3$\sigma$). We measure upper limits of $f_esc$<9.6% from a sample of SFGs selected on high H$\alpha$ equivalent width (EW>200\AA), which are thought to be close analogs of high redshift sources of reionization. For reference, we also present an emissivity--weighted escape fraction which is useful as a measurement of the general contribution of the SFGs to the z~1 ionizing UV background. In the discussion, we consider the implications of these intermediate redshift constraints for the re--ionization of hydrogen in the intergalactic medium at high (z>6) redshift. If the escape fraction of SFGs increases with redshift or an unobserved population of faint (M$_UV$<-13 AB) SFGs with $f_esc$>3% contributes significantly, reionization by SFGs is marginally consistent with independent observations from Planck.

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