An uncontaminated measurement of the escaping Lyman continuum at
arXiv:2104.02081 · doi:10.1093/mnras/stab1374
Abstract
Observations of reionization-era analogs at are a powerful tool for constraining reionization. Rest-ultraviolet observations are particularly useful, in which both direct and indirect tracers of ionizing-photon production and escape can be observed. We analyse a sample of 124 galaxies from the Keck Lyman Continuum Spectroscopic Survey, with sensitive spectroscopic measurements of the Lyman continuum (LyC) region. We present a method of removing foreground contamination from our sample using high-resolution, multiband Hubble Space Telescope imaging. We re-measure the global properties of the cleaned sample of 13 individually-detected LyC sources and 107 individually-undetected sources, including a sample-averaged absolute escape fraction of and a sample-averaged ratio of ionizing to non-ionizing ultraviolet flux density of , corrected for attenuation from the intergalactic and circumgalactic media. Based on composite spectra, we also recover a strong positive correlation between and Ly equivalent width (W(Ly)) and a negative correlation between and UV luminosity. As in previous work, we interpret the relationship between and W(Ly) in terms of the modulation of the escape of ionizing radiation from star-forming galaxies based on the covering fraction of neutral gas. We also use a W(Ly)-weighted to estimate an ionizing emissivity from star-forming galaxies at as erg sHzMpc. This estimate, evaluated using the uncontaminated sample of this work, affirms that the contribution of galaxies to the ionizing background at is comparable to that of active galactic nuclei.
23 pages, 10 figures, accepted for publication in MNRAS
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