High signal-to-noise observations of the Ly α forest transmissivity in the z = 7.085 quasistellar object (QSO) ULAS J1120+0641 show seven narrow transmission spikes followed by a long 240 cMpc h -1 trough. Here, we use radiative transfer simulations of cosmic reionization previously calibrated to match a wider range of Ly α forest data to show that the occurrence of seven transmission spikes in the narrow redshift range z = 5.85-6.1 is very sensitive to the exact timing of reionization. Occurrence of the spikes requires the most underdense regions of the intergalactic medium to be already fully ionized. The rapid onset of a long trough at z = 6.12 requires a strong decrease of the photoionization rate Γ at z ≳ 6.1 in this line of sight, con...
The transmission of Lyman α (Ly α) in the spectra of distant quasars depends on the density, tempera...
The large cross-section of the Lyα line makes it a sensitive probe of the ionization state of the in...
© 2015 The Authors. We report the discovery of an extremely long (~110 Mpc h -1 ) and dark (τ eff ≳...
International audienceHigh signal-to-noise observations of the Ly α forest transmissivity in the z =...
International audienceHigh signal-to-noise observations of the Ly α forest transmissivity in the z =...
High signal-to-noise observations of the Ly α forest transmissivity in the z = 7.085 quasi-stellar o...
We report the discovery of an extremely long (∼110 Mpc/h) and dark (τeff≳7) Lyα trough extending dow...
The presence of excess scatter in the Ly-α forest at z ∼5.5, together with the existence of sporadic...
International audienceA long (110 cMpc ^1) and deep absorption trough in the Ly α forest has been ob...
We present a new investigation of the intergalactic medium (IGM) near the end of reionization using ...
The presence of excess scatter in the Ly-α forest at z ∼ 5.5, together with the existence of sporadi...
It is generally taken for granted that reionization has completed by z = 6, due to the detection of ...
We use numerical simulations to study the effects of the patchiness of a partly reionized inter-gala...
We present a new investigation of the intergalactic medium (IGM) near the end of reionization using ...
Clues about the timing of reionization and the nature of the ionizing sources responsible are imprin...
The transmission of Lyman α (Ly α) in the spectra of distant quasars depends on the density, tempera...
The large cross-section of the Lyα line makes it a sensitive probe of the ionization state of the in...
© 2015 The Authors. We report the discovery of an extremely long (~110 Mpc h -1 ) and dark (τ eff ≳...
International audienceHigh signal-to-noise observations of the Ly α forest transmissivity in the z =...
International audienceHigh signal-to-noise observations of the Ly α forest transmissivity in the z =...
High signal-to-noise observations of the Ly α forest transmissivity in the z = 7.085 quasi-stellar o...
We report the discovery of an extremely long (∼110 Mpc/h) and dark (τeff≳7) Lyα trough extending dow...
The presence of excess scatter in the Ly-α forest at z ∼5.5, together with the existence of sporadic...
International audienceA long (110 cMpc ^1) and deep absorption trough in the Ly α forest has been ob...
We present a new investigation of the intergalactic medium (IGM) near the end of reionization using ...
The presence of excess scatter in the Ly-α forest at z ∼ 5.5, together with the existence of sporadi...
It is generally taken for granted that reionization has completed by z = 6, due to the detection of ...
We use numerical simulations to study the effects of the patchiness of a partly reionized inter-gala...
We present a new investigation of the intergalactic medium (IGM) near the end of reionization using ...
Clues about the timing of reionization and the nature of the ionizing sources responsible are imprin...
The transmission of Lyman α (Ly α) in the spectra of distant quasars depends on the density, tempera...
The large cross-section of the Lyα line makes it a sensitive probe of the ionization state of the in...
© 2015 The Authors. We report the discovery of an extremely long (~110 Mpc h -1 ) and dark (τ eff ≳...