Faint LAEs near z>4.7 CIV absorbers revealed by MUSE
arXiv:2001.04453 · doi:10.1093/mnras/staa3129
Abstract
We present the results from the search for Lyman Alpha emitters (LAEs) in the proximity of 11 CIV absorption systems at in the spectrum of the QSO J1030+0524, using data from MUSE. We have found multiple LAE candidates close to four CIV systems at -5.74 with log(N CIV[cm]) At z = 5-6, CIV systems with W0(CIV) Å seem more likely to have galaxies with Ly emission within proper kpc (4/5 cases), than the CIV systems with W0(CIV) Å (0/6 cases). The impact parameter of LAE-CIV systems with equivalent widths W0(CIV) Å is in the range 11 200 proper kpc (pkpc). Furthermore, all candidates are in the luminosity range 0.18-1.15 L* indicating that the environment of CIV systems within 200 pkpc is populated by the faint end of the Ly luminosity function. We report a 0.28 L* galaxy at a separation of pkpc from a strong CIV absorption (log10(NCIV[cm]) = 14.52) at . The prevalence of sub-L*(Ly) galaxies in the proximity of z CIV systems suggest that the absorbing material is rather young, likely ejected in the recent past of the galaxies at these redshifts. The connection between faint LAEs and high-ionization absorption systems reported in this work, is potentially a consequence of the role of low mass galaxies in the early evolution of the circum-galactic and intergalactic media.
21 pages, 23 figures, 3 tables. Submitted to MNRAS
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