2020MNRAS.498.3095Y

Using a sample of galaxies at z ≃ 3 with detected Lyman Continuum (LyC) leakage in the SSA22 field, we attempt to verify a proposed indirect method for identifying cases with high LyC escape fraction f_esc based on measurements of the H β equivalent width (EW) and the β slope of the UV continuum. To this end, we present Keck/MOSFIRE H β emission line flux measurements of LyC galaxies (LCGs) at spectroscopic redshifts z_spec ∼ 3.3, Lyman break galaxies (LBGs) at photometric redshifts z_phot = 2.7-3.7, and Ly α emitters at z_phot = 3.1. We also reconfirm the spectroscopic redshifts and measure the H β emission-line fluxes from two LCGs and six LBGs. For the LCG in our sample with the most extreme f_esc, as revealed by the direct detection of LyC photons, we find that the EW(H β)-β method gives a broadly consistent estimate for f_esc, although the error bars remain very large. We also discuss how a combination of f_esc measurements based on direct and indirect methods can shed light on the LyC escape mechanism and the anisotropy of the leakage.