The Epoch of Reionization Window: II. Statistical Methods for Foreground Wedge Reduction
arXiv:1404.4372 · doi:10.1103/PhysRevD.90.023019
Abstract
For there to be a successful measurement of the 21 cm Epoch of Reionization (EoR) power spectrum, it is crucial that strong foreground contaminants be robustly suppressed. These foregrounds come from a variety of sources (such as Galactic synchrotron emission and extragalactic point sources), but almost all share the property of being spectrally smooth, and when viewed through the chromatic response of an interferometer, occupy a signature "wedge" region in cylindrical Fourier space. The complement of the foreground wedge is termed the "EoR window", and is expected to be mostly foreground-free, allowing clean measurements of the power spectrum. This paper is a sequel to a previous paper that established a rigorous mathematical framework for describing the foreground wedge and the EoR window. Here, we use our framework to explore statistical methods by which the EoR window can be enlarged, thereby increasing the sensitivity of a power spectrum measurement. We adapt the FKP approximation (commonly used in galaxy surveys) for 21 cm cosmology, and also compare the optimal quadratic estimator to simpler estimators that ignore covariances between different Fourier modes. The optimal quadratic estimator is found to suppress foregrounds by an extra factor of in power at the peripheries of the EoR window, boosting the detection of the cosmological signal from to at the midpoint of reionization in our fiducial models. If numerical issues can be finessed, decorrelation techniques allow the EoR window to be further enlarged, enabling measurements to be made deep within the foreground wedge. These techniques do not assume that foreground are Gaussian-distributed, and we additionally prove that a final round of foreground subtraction can be performed after decorrelation in a way that is guaranteed to have no cosmological signal loss.
19 pages, 8 figures. v2: Updated to match published PRD version. Fixed typos, added figure showing fiducial theoretical model, appendix about Fisher matrices, and detection significance figures in response to referee comments. Main conclusions unchanged
References in corpus (14)
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- How accurately can 21 cm tomography constrain cosmology?
- The Epoch of Reionization Window: I. Mathematical Formalism
- A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
- The Tianlai project: a 21cm cosmology experiment
- The Scale of the Problem : Recovering Images of Reionization with GMCA
- An Improved Method for 21cm Foreground Removal
- Non-parametric foreground subtraction for 21cm epoch of reionization experiments
- Will point sources spoil 21 cm tomography?
- De-contamination of cosmological 21-cm maps
- A Fast Method for Power Spectrum and Foreground Analysis for 21 cm Cosmology
- Higher Order Contributions to the 21 cm Power Spectrum
- The nature of dark matter from the global high redshift HI 21 cm signal
Cited by in corpus (31)
- Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR
- The Epoch of Reionization Window: I. Mathematical Formalism
- 21CMMC: an MCMC analysis tool enabling astrophysical parameter studies of the cosmic 21 cm signal
- First Season MWA EoR Power Spectrum Results at Redshift 7
- Constraining the intergalactic medium at 9.1 using LOFAR Epoch of Reionization observations
- Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
- Visibility based angular power spectrum estimation in low frequency radio interferometric observations
- Spherical Harmonic Analyses of Intensity Mapping Power Spectra
- An Effective Model for the Cosmic-Dawn 21-cm Signal
- Mapmaking for Precision 21 cm Cosmology
- Adding Context to JWST Surveys with Current and Future 21cm Radio Observations
- Exploring the cosmic 21-cm signal from the Epoch of Reionisation using the Wavelet Scattering Transform
- The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
- Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning
- Measuring the growth of structure with intensity mapping surveys
- Constraining Polarized Foregrounds for EOR Experiments II: Polarization Leakage Simulations in the Avoidance Scheme
- Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1
- A Bayesian Calibration Framework for EDGES
- A Tapered Gridded Estimator (TGE) for the Multi-Frequency Angular Power Spectrum (MAPS) and the Cosmological HI 21-cm Power Spectrum
- Measuring HERA's primary beam in-situ: methodology and first results
- Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization
- Exploring the cosmic dawn and epoch of reionization with 21cm line
- On the use of temporal filtering for mitigating galactic synchrotron calibration bias in 21 cm reionization observations
- Probing Compensated Isocurvature with the 21-cm Signal during Cosmic Dawn
- Statistical Detection of IGM Structures during Cosmic Reionization using Absorption of the Redshifted 21 cm line by HI against Compact Background Radio Sources
- Detection of Cosmic Structures using the Bispectrum Phase. I. Mathematical Foundations
- Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator III: Foreground removal
- Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator II: Cross-polarization power spectrum
- Validating a novel angular power spectrum estimator using simulated low frequency radio-interferometric data
- Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
- The Correlation Calibration of PAPER-64 data