Long Dark Gaps in the Ly Forest at : Evidence of Ultra Late Reionization from XQR-30 Spectra
arXiv:2205.04569 · doi:10.3847/1538-4357/ac6e60
Abstract
We present a new investigation of the intergalactic medium (IGM) near reionization using dark gaps in the Lyman- (Ly) forest. With its lower optical depth, Ly offers a potentially more sensitive probe to any remaining neutral gas compared to commonly used Ly line. We identify dark gaps in the Ly forest using spectra of 42 QSOs at , including new data from the XQR-30 VLT Large Programme. Approximately of these QSO spectra exhibit dark gaps longer than at . By comparing the results to predictions from simulations, we find that the data are broadly consistent both with models where fluctuations in the Ly forest are caused solely by ionizing ultraviolet background (UVB) fluctuations and with models that include large neutral hydrogen patches at due to a late end to reionization. Of particular interest is a very long () and dark () gap persisting down to in the Ly forest of the QSO PSO J02511. This gap may support late reionization models with a volume-weighted average neutral hydrogen fraction of by . Finally, we infer constraints on over based on the observed Ly dark gap length distribution and a conservative relationship between gap length and neutral fraction derived from simulations. We find , 0.17, and 0.29 at , 5.75, and 5.95, respectively. These constraints are consistent with models where reionization ends significantly later than .
arXiv comment17 pages, 13 figures, accepted for publication in ApJ. The Figure set and machine readable table are available at https://ydzhuastro.github.io/lyb.html
References in corpus (58)
- Astropy: A Community Python Package for Astronomy
- The NumPy array: a structure for efficient numerical computation
- Planck 2013 results. XVI. Cosmological parameters
- Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ~ 6 Quasars II: A Sample of 19 Quasars
- Radiative transfer in a clumpy universe: IV. New synthesis models of the cosmic UV/X-ray background
- X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope
- An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5
- Model-independent evidence in favor of an end to reionization by z~6
- Evidence of patchy hydrogen reionization from an extreme Ly trough below redshift six
- ESI, a new Keck Observatory echellette spectrograph and imager
- The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly Emission from Galaxies
- Pōniuā'ena: A Luminous Quasar Hosting a 1.5 Billion Solar Mass Black Hole
- Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7
- Hydrogen reionisation ends by : Lyman- optical depth measured by the XQR-30 sample
- Large Lyman-alpha opacity fluctuations and low CMB tau in models of late reionization with large islands of neutral hydrogen extending to z<5.5
- Inferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey
- New constraints on Lyman-α opacity with a sample of 62 quasars at z > 5.7
- A Significantly Neutral Intergalactic Medium Around the Luminous z=7 Quasar J0252-0503
- Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5
- Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium
- Long troughs in the Lyman- forest below redshift 6 due to islands of neutral hydrogen
- The Sherwood simulation suite: overview and data comparisons with the Lyman-alpha forest at redshifts 2 < z < 5
- The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization
- The Opacity of the Intergalactic Medium Measured Along Quasar Sightlines at
- Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman- flux power spectrum
- Texas Spectroscopic Search for Ly Emission at the End of Reionization III. the Ly Equivalent-width Distribution and Ionized Structures at
- Probing the thermal state of the intergalactic medium at with the transmission spikes in high-resolution Ly forest spectra
- Measurements of the z ~ 6 Intergalactic Medium Optical Depth and Transmission Spikes Using a New z > 6.3 Quasar Sample
- Reionization and galaxy inference from the high-redshift Lyα forest
- The Impact of the First Galaxies on Cosmic Dawn and Reionization
- Observing the tail of reionization: neutral islands in the Lyman- Forest
- Approaching Reionization: The Evolution of the Lyman Alpha Forest from Redshifts Four to Six
- The first (nearly) model-independent constraint on the neutral hydrogen fraction at z~5--6
- A consistent and robust measurement of the thermal state of the IGM at from a large sample of Ly forest spectra: Evidence for late and rapid HeII reionization
- Detecting and Characterizing Young Quasars I: Systemic Redshifts and Proximity Zones Measurements
- Glimpsing through the high redshift neutral hydrogen fog
- IGM damping wing constraints on reionisation from covariance reconstruction of two QSOs
- Evidence for Large-Scale Fluctuations in the Metagalactic Ionizing Background Near Redshift Six
- SpectRes: A Fast Spectral Resampling Tool in Python
- Constraining the Topology of Reionization Through Lyman-alpha Absorption
- The Evolution of O I over 3.2 < z < 6.5: Reionization of the Circumgalactic Medium
- Predicting Quasar Continua Near Lyman- with Principal Component Analysis
- Chasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly Forest over
- LAGER Ly Luminosity Function at , Implications for Reionization
- A short mean free path at favors late and rapid reionization by faint galaxies
- The Ly Luminosity Function and Cosmic Reionization at 7.0: a Tale of Two LAGER Fields
- Studying the Lyman- optical depth fluctuations at using fast semi-numerical methods
- Modelling the observed luminosity function and clustering evolution of Lyman- emitters: growing evidence for late reionization
- Inference of the optical depth to reionization from low multipole temperature and polarisation Planck data
- A comparison of quasar emission reconstruction techniques for Lyman- and Lyman- transmission
- Constraining the second half of reionization with the Lyman- forest
- Cosmic Reionization On Computers. Properties of the Post-reionization IGM
- The Predicament of Absorption-Dominated Reionization: Increased Demands on Ionizing Sources
- Determining the Nature of Late Gunn-Peterson Troughs with Galaxy Surveys
- Evidence for a highly opaque large-scale galaxy void at the end of reionization
- Constraints on the End of Reionization from the Density Fields Surrounding Two Highly Opaque Quasar Sightlines
- A Statistical Analysis of Intergalactic Medium Transmission Approaching Reionization
- Anomaly in the Opacity of the Post-Reionization Intergalactic Medium in the Ly and Ly Forest
Cited by in corpus (37)
- EIGER I. a large sample of [OIII]-emitting galaxies at and direct evidence for local reionization by galaxies
- (Nearly) Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at Using Dark Pixel Fractions in Ly and Ly Forests
- XQR-30: the ultimate XSHOOTER quasar sample at the reionization epoch
- Inferring the IGM Neutral Fraction at z ~ 6-8 with Low-Luminosity Lyman Break Galaxies
- Chronicling the reionization history at with emergent quasar damping wings
- Damping Wing-Like Features in the Stacked Ly Forest: Potential Neutral Hydrogen Islands at
- Damping wings in the Lyman-α forest: a model-independent measurement of the neutral fraction at 5.4<z<6.1
- The XQR-30 Metal Absorber Catalog: 778 Absorption Systems Spanning 2 < z < 6.5
- The fraction and kinematics of broad absorption line quasars across cosmic time
- SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
- PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
- Examining the Decline in the C IV Content of the Universe over 4.3 < z < 6.3 using the E-XQR-30 Sample
- The Morphology of Reionization in a Dynamically Clumpy Universe
- LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
- Late-end reionization with ATON-HE: towards constraints from Lyman- emitters observed with JWST
- Optical depth to reionization from perturbative 21cm clustering
- Lyman-alpha Emitters in Ionized Bubbles: Constraining the Environment and Ionized Fraction
- The impact of faint AGN discovered by JWST on reionization
- Probing quasar lifetimes with proximate -centimetre absorption in the diffuse intergalactic medium at redshifts
- Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
- Probing patchy reionisation with JWST: IGM opacity constraints from the Lyman- forest of galaxies in legacy extragalactic fields
- Galaxy Formation and Symbiotic Evolution with the Inter-Galactic Medium in the Age of ELT-ANDES
- The Lyman-limit photon mean free path at the end of late reionisation in the Sherwood-Relics simulations
- Studying the Multi-frequency Angular Power Spectrum of the Cosmic Dawn 21-cm Signal
- Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly emitters and IGM transmission in the COSMOS field at
- Prospects of a statistical detection of the 21-cm forest and its potential to constrain the thermal state of the neutral IGM during reionization
- Impact of the primordial fluctuation power spectrum on the reionization history
- Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
- Ly Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly detection
- Global 21 cm signal: a promising probe of primordial features
- Reionizing islands with inhomogeneous recombinations
- Efficient Modelling of Lyman-α opacity fluctuations during late reionization epoch
- Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography
- Imaging reionization's last phases with I-front Lyman- emissions
- Quantifying Lyman- emissions from reionization fronts
- Efficient neutral-IGM inference from noisy 21-cm forest spectra with latent-space U-Net encoding and XGBoost
- Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations