Intense CIII] 1907,1909 emission from a strong Lyman continuum emitting galaxy
arXiv:1808.03059 · doi:10.1051/0004-6361/201833823
Abstract
We have obtained the first complete ultraviolet (UV) spectrum of a strong Lyman continuum(LyC) emitter at low redshift -- the compact, low-metallicity, star-forming galaxy J1154+2443 -- with a Lyman continuum escape fraction of 46% discovered recently. The Space Telescope Imaging Spectrograph spectrum shows strong Lya and CIII] 1909 emission, as well as OIII] 1666. Our observations show that strong LyC emitters can have UV emission lines with a high equivalent width (e.g. EW(CIII]) rest-frame), although their equivalent widths should be reduced due to the loss of ionizing photons. The intrinsic ionizing photon production efficiency of J1154+2443 is high, erg Hz, comparable to that of other recently discovered LyC emitters. Combining our measurements and earlier determinations from the literature, we find a trend of increasing with increasing CIII] 1909 equivalent width, which can be understood by a combination of decreasing stellar population age and metallicity. Simple ionization and density-bounded photoionization models can explain the main observational features including the UV spectrum of J1154+2443.
arXiv comment5 pages, 4 figures. Accepted for publication in A&A Letters
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