Probing the primordial Universe with MeerKAT and DES
arXiv:1611.01322 · doi:10.1093/mnras/stw3248
Abstract
It is usually assumed that we will need to wait until next-generation surveys like Euclid, LSST and SKA, in order to improve on the current best constraints on primordial non-Gaussianity from the Planck experiment. We show that two contemporary surveys, with the SKA precursor MeerKAT and the Dark Energy Survey (DES), can be combined using the multi-tracer technique to deliver an accuracy on measurement of that is up to three times better than Planck.
arXiv comment7 pages, 5 figures, 1 table. We now marginalise over the bias, and ensure that we exclude nonlinear scales, leading to small quantitative corrections. Version accepted by MNRAS
References in corpus (35)
- Stable clustering, the halo model and nonlinear cosmological power spectra
- Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- The linear power spectrum of observed source number counts
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- What galaxy surveys really measure
- The effect of primordial non-Gaussianity on halo bias
- Measuring primordial non-gaussianity without cosmic variance
- Large-scale clustering of galaxies in general relativity
- Effect of Photometric Redshift Uncertainties on Weak Lensing Tomography
- General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?
- How to measure redshift-space distortions without sample variance
- Minimizing the stochasticity of halos in large-scale structure surveys
- Testing General Relativity with 21 cm intensity mapping
- Redshift distributions of galaxies in the DES Science Verification shear catalogue and implications for weak lensing
- The CLASSgal code for Relativistic Cosmological Large Scale Structure
- Galaxy Clustering and Galaxy Bias in a Lambda-CDM Universe
- Going beyond the Kaiser redshift-space distortion formula: a full general relativistic account of the effects and their detectability in galaxy clustering
- Testing General Relativity on Horizon Scales and the Primordial non-Gaussianity
- Ultra large-scale cosmology in next-generation experiments with single tracers
- Constraining ultra large-scale cosmology with multiple tracers in optical and radio surveys
- Disentangling non-Gaussianity, bias and GR effects in the galaxy distribution
- Hunting down horizon-scale effects with multi-wavelength surveys
- Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
- Why multi-tracer surveys beat cosmic variance
- Radio Galaxy populations and the multi-tracer technique: pushing the limits on primordial non-Gaussianity
- Extending cosmological tests of General Relativity with the Square Kilometre Array
- Einstein's legacy in galaxy surveys
- Cosmological Measurements with General Relativistic Galaxy Correlations
- The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands
- HI and cosmological constraints from intensity mapping, optical, and CMB surveys
- Constraining primordial non-Gaussianity via a multitracer technique with surveys by Euclid and Square Kilometre Array
- Prospects for clustering and lensing measurements with forthcoming intensity mapping and optical surveys
- A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
- The OH line contamination of 21 cm intensity fluctuation measurements for z=1~4
Cited by in corpus (30)
- Fundamental Physics with the Square Kilometre Array
- Line-Intensity Mapping: 2017 Status Report
- Parameter constraints from cross-correlation of CMB lensing with galaxy clustering
- Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
- The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
- Calibrating photometric redshifts with intensity mapping observations
- HI intensity mapping with MeerKAT: 1/f noise analysis
- Simulated multi-tracer analyses with HI intensity mapping
- Disantangling the effects of Doppler velocity and primordial non-Gaussianity in galaxy power spectra
- Synergies between intensity maps of hydrogen lines
- Non-Gaussianity Constraints using Future Radio Continuum Surveys and the Multi-Tracer Technique
- Recovering lost 21 cm radial modes via cosmic tidal reconstruction
- Intensity mapping from the sky: synergizing the joint potential of [OIII] and [CII] surveys at reionization
- Local primordial non-Gaussianity in the relativistic galaxy bispectrum
- Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
- Cross-correlating 21 cm and galaxy surveys: implications for cosmology and astrophysics
- Constraining primordial non-Gaussianity by combining next-generation galaxy and 21 cm intensity mapping surveys
- Multi-tracer power spectra and bispectra: Formalism
- Constraining the growth rate by combining multiple future surveys
- Beyond CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
- Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
- Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- III. Implementing the multi-tracer technique to constrain neutrino masses
- A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
- Unveiling the Universe with Emerging Cosmological Probes
- Decoupling Local Primordial non-Gaussianity from Relativistic Effects in the Galaxy Bispectrum
- Probing Quintessence using BAO imprint on the cross-correlation of weak lensing and post-reionization HI 21 cm signal
- Constraining primordial non-Gaussianity by combining photometric galaxy and 21cm intensity mapping surveys
- Squeezing information from radio surveys to probe the primordial Universe
- Multi-wavelength spectroscopic probes: prospects for primordial non-Gaussianity and relativistic effects
- Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx