Distinguishing models of reionization using future radio observations of 21-cm 1-point statistics
arXiv:1312.1342 · doi:10.1093/mnras/stu1384
Abstract
We explore the impact of reionization topology on 21-cm statistics. Four reionization models are presented which emulate large ionized bubbles around over-dense regions (21CMFAST/ global-inside- out), small ionized bubbles in over-dense regions (local-inside-out), large ionized bubbles around under-dense regions (global-outside-in) and small ionized bubbles around under-dense regions (local-outside-in). We show that first-generation instruments might struggle to distinguish global models using the shape of the power spectrum alone. All instruments considered are capable of breaking this degeneracy with the variance, which is higher in outside-in models. Global models can also be distinguished at small scales from a boost in the power spectrum from a positive correlation between the density and neutral-fraction fields in outside-in models. Negative skewness is found to be unique to inside-out models and we find that pre-SKA instruments could detect this feature in maps smoothed to reduce noise errors. The early, mid and late phases of reionization imprint signatures in the brightness-temperature moments, we examine their model dependence and find pre-SKA instruments capable of exploiting these timing constraints in smoothed maps. The dimensional skewness is introduced and is shown to have stronger signatures of the early and mid-phase timing if the inside-out scenario is correct.
arXiv comment18 pages, 13 figures, updated to agree with published version
References in corpus (63)
- Planck 2013 results. XVI. Cosmological parameters
- Large scale bias and the peak background split
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Mass function of dark matter halos
- A luminous quasar at a redshift of z = 7.085
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ~ 6 Quasars II: A Sample of 19 Quasars
- In the Beginning: The First Sources of Light and the Reionization of the Universe
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- 21-cm cosmology
- Evidence for Reionization at z ~ 6: Detection of a Gunn-Peterson Trough in a z=6.28 Quasar
- 21-cm Tomography of the Intergalactic Medium at High Redshift
- 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
- The Growth of HII Regions During Reionization
- New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign
- Evolution of the Ionizing Background and the Epoch of Reionization from the Spectra of z~6 Quasars
- Reionization of the Inhomogeneous Universe
- Reionization and Cosmology with 21 cm Fluctuations
- Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization
- Efficient Simulations of Early Structure Formation and Reionization
- 21 Centimeter Fluctuations from Cosmic Gas at High Redshifts
- The Radiative Feedback of the First Cosmological Objects
- Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844 - 7.213: Demographics of Lyman-Alpha Emission in z ~ 7 Galaxies
- Bright Source Subtraction Requirements For Redshifted 21 cm Measurements
- What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization
- Reionization and the Cosmic Dawn with the Square Kilometre Array
- Spectroscopic confirmation of z~7 LBGs: probing the earliest galaxies and the epoch of reionization
- Keck Spectroscopy of Faint 3<z<8 Lyman Break Galaxies:- Evidence for a Declining Fraction of Emission Line Sources In the Redshift Range 6<z<8
- 21 cm fluctuations from inhomogeneous X-ray heating before reionization
- Photoionization Feedback in Low--Mass Galaxies at High Redshift
- Taxing the Rich: Recombinations and Bubble Growth During Reionization
- How neutral is the intergalactic medium surrounding the redshift z=7.085 quasar ULAS J1120+0641?
- A lower limit of dz > 0.06 for the duration of the reionization epoch
- Simulating Cosmic Reionization at Large Scales II: the 21-cm Emission Features and Statistical Signals
- Statistical Probes of Reionization With 21 cm Tomography
- The impact of point source subtraction residuals on 21 cm Epoch of Reionization estimation
- Evolution of the 21 cm signal throughout cosmic history
- Simulating cosmic reionization: How large a volume is large enough?
- Constraints on reionization from the thermal history of the intergalactic medium
- Foreground Contamination in Interferometric Measurements of the Redshifted 21 cm Power Spectrum
- MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey
- Constraining the unexplored period between reionization and the dark ages with observations of the global 21 cm signal
- Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array
- Twenty-one centimeter tomography with foregrounds
- A Measurement of Small Scale Structure in the 2.2 < z < 4.2 Lyman-alpha Forest
- On the Evolution of the Ionizing Emissivity of Galaxies and Quasars Required by the Hydrogen Reionization
- Topology and Sizes of HII Regions during Cosmic Reionization
- Lyman Alpha Emitters at z=7 in the Subaru/XMM-Newton Deep Survey Field: Photometric Candidates and Luminosity Function
- UV Radiative Feedback During the Advanced Stages of Reionization
- The visibility of Lyman Alpha Emitters during reionization
- A first direct measurement of the intergalactic medium temperature around a quasar at z=6
- Systematic Effects of Foreground Removal in 21cm Surveys of Reionization
- Global 21cm signal experiments: A designer's guide
- Biased Reionisation and Non-Gaussianity in Redshifted 21cm Intensity Maps of the Reionisation Epoch
- Detection and extraction of signals from the epoch of reionization using higher order one-point statistics
- On the minimum mass of reionization sources
- Imaging neutral hydrogen on large-scales during the Epoch of Reionization with LOFAR
- The Difference PDF of 21-cm Fluctuations: A Powerful Statistical Tool for Probing Cosmic Reionization
- Measuring the History of Cosmic Reionization using the 21-cm PDF from Simulations
- Measuring the Redshift of Reionization with a Modest Array of Low-Frequency Dipoles
- Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
- Measuring the History of Cosmic Reionization using the 21-cm Difference PDF
- Luminosity Functions and Star Formation Rates at z~6-10: Galaxy Buildup in the Reionization Age
Cited by in corpus (51)
- Upper limits on the 21-cm Epoch of Reionization power spectrum from one night with LOFAR
- Data Analysis for Precision 21 cm Cosmology
- Eliminating the optical depth nuisance from the CMB with 21 cm cosmology
- CHIPS: The Cosmological HI Power Spectrum Estimator
- Quantifying the non-Gaussianity in the EoR 21-cm signal through bispectrum
- The Rise of the First Stars: Supersonic Streaming, Radiative Feedback, and 21-cm Cosmology
- Bubble size statistics during reionization from 21-cm tomography
- Optimal identification of HII regions during reionization in 21-cm observations
- The 21cm bispectrum as a probe of non-Gaussianities due to X-ray heating
- 21cm-line bispectrum as method to probe Cosmic Dawn and Epoch of Reionization
- Constraining the epoch of reionization with the variance statistic: simulations of the LOFAR case
- A fast estimator for the bispectrum and beyond - A practical method for measuring non-Gaussianity in 21-cm maps
- The Large-Scale Observational Signatures of Low-Mass Galaxies During Reionization
- Constraining the EoR model parameters with the 21cm bispectrum
- Position-dependent power spectra of the 21-cm signal from the epoch of reionization
- The impact of spin temperature fluctuations on the 21-cm moments
- Statistics of the epoch of reionization 21-cm signal - I. Power spectrum error-covariance
- Studying 21cm power spectrum with one-point statistics
- Redshifted 21-cm Bispectrum I: Impact of the Redshift Space Distortions on the Signal from the Epoch of Reionization
- Stages of Reionization as revealed by the Minkowski Functionals
- Exploring the cosmic 21-cm signal from the Epoch of Reionisation using the Wavelet Scattering Transform
- Redshifted 21-cm bispectrum II: Impact of the spin temperature fluctuations and redshift space distortions on the signal from the Cosmic Dawn
- Effects of the sources of reionization on 21-cm redshift-space distortions
- Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
- Models of the Cosmological 21 cm Signal from the Epoch of Reionization Calibrated with Lyman-alpha and CMB Data
- Dark-ages reionization & galaxy formation simulation V: morphology and statistical signatures of reionization
- Inferring the properties of the sources of reionization using the morphological spectra of the ionized regions
- Detection of Cosmic Structures using the Bispectrum Phase. II. First Results from Application to Cosmic Reionization Using the Hydrogen Epoch of Reionization Array
- The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability
- Expected constraints on models of the epoch of reionization with the variance and skewness in redshifted 21cm-line fluctuations
- Reionisation & Cosmic Dawn Astrophysics from the Square Kilometre Array: Impact of Observing Strategies
- Bayesian Model Selection with Future 21cm Observations of The Epoch of Reionisation
- Constraining the Epoch of Reionization With Highly Dispersed Fast Radio Bursts
- Exploring the cosmic dawn and epoch of reionization with 21cm line
- Detecting the non-Gaussianity of the 21-cm signal during reionisation with the Wavelet Scattering Transform
- Probing early universe through redshifted 21-cm signal: Modelling and observational challenges
- Quantifying Density-Ionization Correlations with the 21cm Power Spectrum
- Detectability of 21cm-signal during the Epoch of Reionization with 21cm-Lyman-α emitter cross-correlation. II. Foreground contamination
- Sensitivity of the Hydrogen Epoch of Reionization Array and its Build-out Stages to One-point Statistics from Redshifted 21 cm Observations
- 21-cm signatures of residual HI inside cosmic HII regions during reionization
- Persistent topology of the reionization bubble network. II: Evolution & Classification
- Statistical Detection of IGM Structures during Cosmic Reionization using Absorption of the Redshifted 21 cm line by HI against Compact Background Radio Sources
- Redshifted 21-cm bispectrum: Impact of the source models on the signal and the IGM physics from the Cosmic Dawn
- Quantiles as Robust Probes of Non-Gaussianity in 21-cm Images
- Using the sample variance of 21cm maps as a tracer of the ionisation topology
- Lyman Alpha Emitters and the 21cm Power Spectrum as Probes of Density-Ionization Correlation in the Epoch of Reionization
- Impact of the Epoch of Reionization sources on the 21-cm bispectrum
- Measurements of one-point statistics in 21 cm intensity maps via foreground avoidance strategy
- Reionization and Cosmic Dawn: theory and simulations
- Impact of astrophysical scatter on the Epoch of Reionization [H I] bispectrum
- Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-Point Statistics