A unique window into the Epoch of Reionisation: A double-peaked Lyman- emitter in the proximity zone of a quasar at
arXiv:2412.12256 · doi:10.1051/0004-6361/202453469
Abstract
We present a study of a double-peaked Ly emitter, named LAE-11, found in the proximity zone of QSO J0910-0414 at . We use a combination of deep photometric data from Subaru Telescope, HST, and JWST with spectroscopic data from Keck/DEIMOS, NIRCam WFSS and NIRSpec MSA to characterise the ionising and general properties of the galaxy, as well as the quasar environment surrounding it. We detect Ly, H, [OIII] doublet, and H emission lines in the various spectral datasets. The presence of a double-peaked Ly line in the spectrum allows us to characterise the opening angle and lifetime of the QSO as ° and years. LAE-11 is a fairly bright (M$_\rm{UV} = -19.84^{+0.14}_{-0.16}$), blue galaxy with a UV slope of . Since the galaxy is located in a quasar-ionised region, we have a unique opportunity to measure the escape fraction of Lyman Continuum photons using the un-attenuated double-peaked Ly emission profile and its equivalent width at such high redshift. We employ diagnostics which do not rely on the detection of Ly for comparison, and find that all tracers of ionising photon leakage agree within 1 uncertainty. We measure a moderate escape of Lyman Continuum photons from LAE-11 of $f_\rm{esc}^\rm{LyC} = (8 - 33)\%$. Detections of both H and H emission lines allow for separate measurements of the ionising photon production efficiency, resulting with $\log(ξ_\rm{ion}/\rm{Hz~erg^{-1}}) = 25.59\pm0.08$ and , for H and H, respectively. The total ionising output of LAE-11, $\log(f_\rm{esc}^\rm{LyC}ξ_\rm{ion, Hα}/\rm{Hz~erg^{-1}}) = 24.85^{+0.24}_{-0.34}$, is higher than the value of which is traditionally assumed as needed to drive Reionisation forward.
Submitted to A&A. Abstract abridged for arxiv
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