2021MNRAS.503.1734I

We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of nine low-mass star-forming galaxies at redshifts, z, in the range 0.3179-0.4524, with stellar masses M_* < 10⁸ M_☉ and very high specific star-formation rates sSFR ∼150-630 Gyr^–1, aiming to study the dependence of leaking Lyman continuum (LyC) emission on stellar mass and some other characteristics of the galaxy. We detect LyC emission in four out of nine galaxies with escape fractions, f_esc(LyC), in the range of 11-35 per cent, and establish upper limits for f_esc(LyC) in the remaining five galaxies. We observe a narrow Ly α emission line with two peaks in seven galaxies and likely more complex Ly α profiles in the two remaining galaxies. The velocity separation between the peaks V_sep varies in the range from ∼229 to ∼512 km s^–1. Our additional data on low-mass galaxies confirm and strengthen the tight anticorrelation between f_esc(LyC) and V_sep found for previous low-redshift galaxy samples with higher stellar masses. V_sep remains the best indirect indicator of LyC leakage. It is better than O₃₂ on which f_esc(LyC) depends weakly, with a large scatter. Finally, contrary to expectations, we find no increase of f_esc(LyC) with decreasing galaxy stellar mass M_*.