The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
arXiv:2302.07034 · doi:10.1093/mnras/stad1567
Abstract
Blind cleaning methods are currently the preferred strategy for handling foreground contamination in single-dish HI intensity mapping surveys. Despite the increasing sophistication of blind techniques, some signal loss will be inevitable across all scales. Constructing a corrective transfer function using mock signal injection into the contaminated data has been a practice relied on for HI intensity mapping experiments. However, assessing whether this approach is viable for future intensity mapping surveys where precision cosmology is the aim, remains unexplored. In this work, using simulations, we validate for the first time the use of a foreground transfer function to reconstruct power spectra of foreground-cleaned low-redshift intensity maps and look to expose any limitations. We reveal that even when aggressive foreground cleaning is required, which causes negative bias on the largest scales, the power spectrum can be reconstructed using a transfer function to within sub-percent accuracy. We specifically outline the recipe for constructing an unbiased transfer function, highlighting the pitfalls if one deviates from this recipe, and also correctly identify how a transfer function should be applied in an auto-correlation power spectrum. We validate a method that utilises the transfer function variance for error estimation in foreground-cleaned power spectra. Finally, we demonstrate how incorrect fiducial parameter assumptions (up to bias) in the generation of mocks, used in the construction of the transfer function, do not significantly bias signal reconstruction or parameter inference (inducing bias in recovered values).
arXiv comment25 pages, 20 figures. See Figure 4 for the main demonstration of the transfer function's performance for reconstructing signal loss from foreground cleaning. Accepted for publication in MNRAS
References in corpus (70)
- Planck 2015 results. XIII. Cosmological parameters
- Efficient Computation of CMB anisotropies in closed FRW models
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Acoustic Signatures in the Primary Microwave Background Bispectrum
- MultiDark simulations: the story of dark matter halo concentrations and density profiles
- Power Spectrum Analysis of Three-Dimensional Redshift Surveys
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
- Single field consistency relation for the 3-point function
- The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation
- Constraints on local primordial non-Gaussianity from large scale structure
- The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
- Fundamental Physics with the Square Kilometre Array
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- Solving Large Scale Structure in Ten Easy Steps with COLA
- Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
- Multifrequency analysis of 21 cm fluctuations from the Era of Reionization
- Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
- Determination of z~0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping auto-correlation
- HI intensity mapping : a single dish approach
- Towards a free-free template for CMB foregrounds
- The Epoch of Reionization Window: II. Statistical Methods for Foreground Wedge Reduction
- Foreground Removal using FastICA: A Showcase of LOFAR-EoR
- Lack of clustering in low-redshift 21-cm intensity maps cross-correlated with 2dF galaxy densities
- Constraining primordial non-Gaussianity with future galaxy surveys
- Baryonic Acoustic Oscillations in 21cm Emission: A Probe of Dark Energy out to High Redshifts
- Blind foreground subtraction for intensity mapping experiments
- Neutral hydrogen surveys for high redshift galaxy clusters and proto-clusters
- Ultra large-scale cosmology in next-generation experiments with single tracers
- Foregrounds for 21cm Observations of Neutral Gas at High Redshift
- The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
- Hunting down horizon-scale effects with multi-wavelength surveys
- Using HI to probe large scale structures at z ~ 3
- HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies
- HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
- The effect of foreground subtraction on cosmological measurements from Intensity Mapping
- Cosmology on Ultralarge Scales with Intensity Mapping of the Neutral Hydrogen 21 cm Emission: Limits on Primordial Non-Gaussianity
- Extending cosmological tests of General Relativity with the Square Kilometre Array
- Interpreting the unresolved intensity of cosmologically redshifted line radiation
- Einstein's legacy in galaxy surveys
- HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations
- MultiDark-Galaxies: data release and first results
- Fast simulations for intensity mapping experiments
- Characterizing Signal Loss in the 21 cm Reionization Power Spectrum: A Revised Study of PAPER-64
- SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
- Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
- 21cm foregrounds and polarization leakage: a user's guide on cleaning and mitigation strategies
- Recovery of 21 cm intensity maps with sparse component separation
- deep21: a Deep Learning Method for 21cm Foreground Removal
- Reconstructing large-scale structure with neutral hydrogen surveys
- Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
- Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
- Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
- HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
- Observational signatures of modified gravity on ultra-large scales
- HI intensity mapping with MeerKAT: 1/f noise analysis
- Simulated multi-tracer analyses with HI intensity mapping
- Gaussian Process Regression for foreground removal in HI intensity mapping experiments
- The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
- Power spectrum modelling of galaxy and radio intensity maps including observational effects
- Detecting the power spectrum turnover with HI intensity mapping
- Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
- The HI intensity mapping bispectrum including observational effects
- Constraints on Primordial non-Gaussianity from Future HI Intensity Mapping Experiments
- Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
- Measuring ultra-large scale effects in the presence of 21cm intensity mapping foregrounds
- Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
- Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
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- Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator III: Foreground removal
- Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
- 21-cm foreground removal using AI and frequency-difference technique
- Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experiment
- Radio-optical synergies at high redshift to constrain primordial non-Gaussianity
- SIMPLE: Simple Intensity Map Producer for Line Emission
- Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
- A wide-angle formulation of foreground filters for HI intensity mapping
- Constraining primordial non-Gaussianity by combining photometric galaxy and 21cm intensity mapping surveys
- Multi-tracing the primordial Universe with future surveys
- Primary Beam Chromaticity in HIRAX: I. Characterization from Simulations and Power Spectrum Implications
- Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
- Squeezing information from radio surveys to probe the primordial Universe
- Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
- HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
- A quadratic estimator view of the transfer function correction in intensity mapping surveys
- Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
- Mitigating gain calibration errors from EoR observations with SKA1-Low AA*
- Foreground Subtraction with a Tensor-Based Oriented Singular Value Decomposition Method for HI Experiments