Observations of the Lyman series forest towards the redshift 7.1 quasar ULAS J1120+0641

Abstract

We present a 30h integration Very Large Telescope X-shooter spectrum of the Lyman series forest towards the $z=7.084$ quasar ULAS J1120+0641. The only detected transmission at $S/N>5$ is confined to seven narrow spikes in the Ly$\alpha$ forest, over the redshift range $5.858<z<6.122$, just longward of the wavelength of the onset of the Ly$\beta$ forest. There is also a possible detection of one further unresolved spike in the Ly$\beta$ forest at $z=6.854$, with $S/N=4.5$. We also present revised Hubble Space Telescope F814W photometry of the source. The summed flux from the transmission spikes is in agreement with the F814W photometry, so all the transmission in the Lyman series forest may have been detected. There is a Gunn-Peterson (GP) trough in the Ly$\alpha$ forest from $z=6.122$ all the way to the quasar near zone at $z=7.04$. The trough, of comoving length $240h^{-1}$Mpc, is over twice as long as the next longest known GP trough. We combine the spectroscopic and photometric results to constrain the evolution of the Ly$\alpha$ effective optical depth with redshift, ${\tau }_{\mathrm{GP}}^{\mathrm{eff}}$ extending a similar analysis by Simpson et al. We find ${\tau }_{\mathrm{GP}}^{\mathrm{eff}}\propto (1+z{)}^{\xi }$ where $\xi =11.2_{-0.6}^{+0.4}$, for $z>5.5$. The data nevertheless provide only a weak limit on the volume-weighted hydrogen intergalactic (IGM) neutral fraction at $z\sim 6.5$, $x_{\mathrm{HI}}>10^{-4}$, similar to limits at redshift $z\sim 6$ from less distant quasars. The new observations cannot extend measurements of the neutral fraction of the IGM to higher values because absorption in the Ly$\alpha$ forest is already saturated near $z\sim 6$. For higher neutral fractions, other methods such as measuring the red damping wing of the IGM will be required.

Accepted for publication in A&A. 11 pages, 10 figures

References in corpus (7)

• A luminous quasar at a redshift of z = 7.085
• Observational constraints on Cosmic Reionization
• Model-independent evidence in favor of an end to reionization by z~6
• The first ultraviolet quasar stacked spectrum at z=2.4 from WFC3
• Extremely metal-poor gas at a redshift of 7
• No excess of bright galaxies around the redshift 7.1 quasar ULAS J1120+0641
• The spectral energy distribution of the redshift 7.1 quasar ULAS J1120+0641

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