2020/12/31 by Kirill Makan, Gábor Worseck, Frederick B. Davies +3 · 25 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Intergalactic medium #Intergalactic travel #Ionization #Photoionization #Quasar #Redshift #Reionization #Spectral line #Transmission (telecommunications) #astro-ph.CO
paper · pdf · doi:10.3847/1538-4357/abee17
published in The Astrophysical Journal 912(1), 38 (IOP Publishing) · Accepted for publication in ApJ following minor revision; 21 pages, 17 figures
openalex created_date 2020/12/21 · arxiv created 2021/03/11 · openalex publication_date 2021/05/01 · arxiv updated 2021/05/06 · openalex updated_date 2026/08/06
Abstract We present new high-resolution ( R = λ /Δ λ ∼ 14,000) spectra of the two brightest He ii -transparent quasars in the far-UV at z em > 3.5, HE2QS J2311−1417 ( z em = 3.70) and HE2QS J1630+0435 ( z em = 3.81), obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope. In the predominantly saturated He ii absorption spectra, both sight lines show several isolated resolved (FWHM ≳ 50 km s −1 ) transmission spikes in He ii Ly α and He ii Ly β . The incidence of such spikes decreases with increasing redshift, but both sight lines show significant spikes at z ≳ 3.5, signaling the presence of fully ionized regions in the z ≳ 3.5 intergalactic medium (IGM). We employ an automated algorithm to compare the number of detected He ii transmission spikes to predictions from mock spectra created from the outputs of a cubic (146 cMpc) 3 optically thin Nyx hydrodynamical simulation, assuming a range of UV background photoionization rates Γ He II . From the incidence of Ly α and Ly β transmission spikes we infer similar photoionization rates of at 3.51 < z < 3.66 and Γ He II = (0.9 ± 0.3) × 10 −15 s −1 at 3.460 < z < 3.685, respectively. Because the transmission spikes indicate fully ionized regions at z ≳ 3.5 along both lines of sight, our observations provide further evidence that He ii reionization had substantially progressed at these redshifts.