HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck

Abstract

The 21 cm emission from neutral hydrogen surveys holds great potential as a valuable method for exploring the large-scale structure of the Universe. In this paper, we forecast for the cross-correlation between the Thermal Sunyaev-Zel'dovich (SZ) fluctuations as probed by the Planck satellite, and fluctuations in the HI brightness temperature as probed by the ground-based Five-hundred-meter Aperture Spherical Telescope (FAST), to trace the connection between galaxy clusters and the HI large-scale structure. Assuming that the measurement is limited by instrumental noise rather than by foreground, we estimate the potential detectability of the cross-correlation signal and their improvement in the measurement of the HI cosmic density, the hydrostatic mass bias parameter, and the universal pressure profile (UPP) parameters. We obtain a constraint on the cosmic neutral hydrogen density parameter significantly to $\sigma ({\Omega }_{\mathrm{HI}})=1.0\times 10^{-6}$. We also find that the average halo masses contributing to the $\mathrm{HI}-y$ cross-power spectrum in the one-halo regime is $\sim 1.5\times 10^{14}{M}_{\odot }$. Our results also show that the HI-SZ cross-correlation has great potential to probe the distribution of neutral hydrogen (HI) within halos at low redshift.

18 pages, 4 figures, 3 tables, accepted in the Astrophysical Journal

References in corpus (112)

• Halo Models of Large Scale Structure
• Cosmology with the Sunyaev-Zel'dovich Effect
• The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
• The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
• Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium
• Concentration, Spin and Shape of Dark Matter Haloes: Scatter and the Dependence on Mass and Environment
• The WiggleZ Dark Energy Survey: Survey Design and First Data Release
• The Sunyaev-Zel'dovich angular power spectrum as a probe of cosmological parameters
• The HIPASS catalogue: Omega_HI and environmental effects on the HI mass function of galaxies
• Damped Lyman Alpha Systems at z<1.65: The Expanded SDSS HST Sample
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function at z < 0.06
• Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
• The Fundamental Performance of FAST with 19-beam Receiver at L Band
• Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
• Column density distribution and cosmological mass density of neutral gas: Sloan Digital Sky Survey-III Data Release 9
• On the (Non)Evolution of HI Disks over Cosmic Time
• Considerations for a Multi-beam Multi-purpose Survey with FAST
• The Arecibo Legacy Fast ALFA Survey: X. The HI Mass Function and Omega_HI From the 40% ALFALFA Survey
• Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7
• How accurately can 21 cm tomography constrain cosmology?
• Determination of z~0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping auto-correlation
• The Atacama Cosmology Telescope: The polarization-sensitive ACTPol instrument
• HI intensity mapping : a single dish approach
• The evolution of Omega(HI) and the epoch of formation of damped Lyman-alpha absorbers
• Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
• On the Cluster Physics of Sunyaev-Zel'dovich Surveys II: Deconstructing the Thermal SZ Power Spectrum
• Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
• A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
• Lack of clustering in low-redshift 21-cm intensity maps cross-correlated with 2dF galaxy densities
• HIRAX: A Probe of Dark Energy and Radio Transients
• The ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass Density
• The HI content of star-forming galaxies at z = 0.24
• Testing General Relativity with 21 cm intensity mapping
• Twenty-one centimeter tomography with foregrounds
• The Tianlai project: a 21cm cosmology experiment
• Predictions for ASKAP Neutral Hydrogen Surveys
• The large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest: First Measurements from BOSS
• Detection of HI in distant galaxies using spectral stacking
• Cosmological evolution of atomic gas and implications for 21 cm HI absorption
• The Scale of the Problem : Recovering Images of Reionization with GMCA
• An observational and theoretical view of the radial distribution of HI gas in galaxies
• A ground-based 21cm Baryon acoustic oscillation survey
• The Five-hundred-meter Aperture Spherical Radio Telescope (FAST) Project
• 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
• HI as a Probe of the Large Scale Structure in the Post-Reionization Universe
• Neutral atomic hydrogen (HI) gas evolution in field galaxies at z ~ 0.1 and 0.2
• A Virtual Sky with Extragalactic HI and CO Lines for the SKA and ALMA
• Cosmology on Ultralarge Scales with Intensity Mapping of the Neutral Hydrogen 21 cm Emission: Limits on Primordial Non-Gaussianity
• Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array
• A halo model for cosmological neutral hydrogen: abundances and clustering
• HI 21-centimetre emission from an ensemble of galaxies at an average redshift of one
• Neutral hydrogen (HI) gas content of galaxies at $z\approx 0.32$
• The FAST all sky HI survey (FASHI): The first release of catalog
• Cosmology from the Thermal Sunyaev-Zel'dovich Power Spectrum: Primordial non-Gaussianity and Massive Neutrinos
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• The First Observations of Low Redshift Damped Lyman-alpha Systems with the Cosmic Origins Spectrograph
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• Weighing neutrinos with cosmic neutral hydrogen
• CMB/kSZ and Compton-$y$ Maps from 2500 square degrees of SPT-SZ and Planck Survey Data
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Atomic hydrogen in star-forming galaxies at intermediate redshifts
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Modelling neutral hydrogen in galaxies using cosmological hydrodynamical simulations
• Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
• Impact of Foregrounds on HI Intensity Mapping Cross-Correlations with Optical Surveys
• Statistical properties of damped Lyman-alpha systems from Sloan Digital Sky Survey DR12
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• A Comparison and Joint Analysis of Sunyaev-Zel'dovich Effect Measurements from Planck and Bolocam for a set of 47 Massive Galaxy Clusters
• Simulated multi-tracer analyses with HI intensity mapping
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• The ALMA REBELS Survey: The Cosmic HI Gas Mass Density in Galaxies at $z\approx 7$
• Cross-correlation of the thermal Sunyaev-Zel'dovich effect and weak gravitational lensing: Planck and Subaru Hyper Suprime-Cam first-year data
• Intensity mapping cross-correlations II: HI halo models including shot noise
• The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
• Damped Lyman-alpha Absorbers from Sloan Digital Sky Survey DR16Q with Gaussian processes
• Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
• Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
• Detecting neutral hydrogen in emission at redshift z ~ 1
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• The evolution of neutral hydrogen over the past 11 Gyr via HI 21 cm absorption
• Detecting the power spectrum turnover with HI intensity mapping
• MIGHTEE-HI: The first MeerKAT HI mass function from an untargeted interferometric survey
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• PACT. II. Pressure profiles of galaxy clusters using Planck and ACT
• Cross-correlating 21 cm and galaxy surveys: implications for cosmology and astrophysics
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Optimization Study for the Experimental Configuration of CMB-S4
• The Tianlai dish array low-z surveys forecasts
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen
• Joint measurement of the galaxy cluster pressure profile with Planck and SPT-SZ
• Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
• Recovering 21-cm signal from simulated FAST intensity maps
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• CMBR Weak Lensing and HI 21-cm Cross-correlation Angular Power Spectrum
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• Probing the cluster pressure profile with thermal Sunyaev-Zeldovich effect and weak lensing cross-correlation
• Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator -- IV. Wideband analysis
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• Detectability of the ${\tau }_{es}$-21cm cross-correlation: a tomographic probe of patchy reionization
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Reconstructing the Long-wavelength Matter Density Fluctuation Modes from the Scalar-Type Clustering Fossils