Prospects for clustering and lensing measurements with forthcoming intensity mapping and optical surveys
arXiv:1509.03286 · doi:10.1093/mnras/stw658
Abstract
We explore the potential of using intensity mapping surveys (MeerKAT, SKA) and optical galaxy surveys (DES, LSST) to detect HI clustering and weak gravitational lensing of 21cm emission in auto- and cross-correlation. Our forecasts show that high precision measurements of the clustering and lensing signals can be made in the near future using the intensity mapping technique. Such studies can be used to test the intensity mapping method, and constrain parameters such as the HI density , the HI bias and the galaxy-HI correlation coefficient .
9 pages, 8 figures, matches version accepted for publication in MNRAS
References in corpus (11)
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- Late-time cosmology with 21cm intensity mapping experiments
- How accurately can 21 cm tomography constrain cosmology?
- Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
- The Neutral Hydrogen Cosmological Mass Density at z=5
- Extending cosmological tests of General Relativity with the Square Kilometre Array
- Simulations for single-dish intensity mapping experiments
- The evolution of neutral gas in damped Lyman systems from the XQ-100 survey
- Weighing neutrinos with cosmic neutral hydrogen
- Dependence of the bright end of galaxy luminosity function on cluster dynamical state
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- Intensity Mapping as a Probe of Axion Dark Matter
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- Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
- Simulated multi-tracer analyses with HI intensity mapping
- Lensing reconstruction from line intensity maps: the impact of gravitational nonlinearity
- Probing the primordial Universe with MeerKAT and DES
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- Recovering lost 21 cm radial modes via cosmic tidal reconstruction
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- Testing gravity at large scales with HI intensity mapping
- Cross-correlating 21 cm and galaxy surveys: implications for cosmology and astrophysics
- HI Intensity Mapping for Clustering-Based Redshift Estimation
- Beyond CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
- Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
- Intensity mapping of the 21cm emission: lensing
- Testing gravity with gravitational waves electromagnetic probes cross-correlations
- A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing
- Simulations for 21 cm radiation lensing at EoR redshifts
- The gravitational and lensing-ISW bispectrum of 21cm radiation
- Unveiling the Universe with Emerging Cosmological Probes
- A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
- Cross-correlation of the Polarizations of the 21-cm and Cosmic Microwave Backgrounds
- Axion-like particle searches with MeerKAT and SKA
- Differentiating Warm Dark Matter Models through 21cm Line Intensity Mapping: A Convolutional Neural Network Approach
- Sensitivity toward dark matter annihilation imprints on 21-cm signal with SKA-Low: A convolutional neural network approach