Unraveling the Lyman Continuum Emission of Ion3: Insights from HST multi-band imaging and X-Shooter spectroscopy
arXiv:2504.18711 · doi:10.1051/0004-6361/202451959
Abstract
We provide a comprehensive analysis of Ion3, the most distant LyC leaker at , using multi-band HST photometry and X-Shooter spectroscopy. Deep HST F390W imaging probe uncontaminated LyC flux blueward 880Å, while the non-ionizing UV 1500Å/2800Å~flux is probed with the F814W/F140W band. High angular resolution allows us to properly mask low- interlopers and prevent contamination of measured LyC radiation. We confirm the detection of LyC flux at SNR 3.5 and estimate the escape fraction of ionizing photons to be in the range = 0.06 -- 1, depending on the adopted IGM attenuation. Morphological analysis reveals a clumpy structure made of two main components, with effective radii of R 180 pc and R < 100 pc, and a total estimated de-lensed area in the rest-frame 1600Å~of 4.2~kpc. We confirm the presence of faint ultraviolet spectral features HeII1640, CIII]1907,1909 and [NeIII]3968, with rest-frame EW(HeII) = (1.60.7)Å and EW(CIII]) = (6.53)Å. From [OII]3726,3729 and [CIII]1909/CIII]1906 we derive electron densities = 23001900 cm and > 10 cm, corresponding to an ISM pressure log(P/k) > 7.90. Furthermore, we derive an intrinsic SFR(H) 77 M yr (corresponding to ~M~yr~kpc for the entire galaxy) and sub-solar metallicity = 8.020.20 using the EW(CIII]) as a diagnostic. The detection of [NeIII]3968 line and [OII]3726,3729, provide an estimate of the ratio [OIII]5007/[OII]3727,29 of O32 > 50 and high ionization parameter log > 1.5 using empirical and theoretical correlations.
12 pages, 12 figures, Accepted to A&A
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