A User's Guide to Extracting Cosmological Information from Line-Intensity Maps
arXiv:1907.10067 · doi:10.1103/PhysRevD.100.123522
Abstract
Line-intensity mapping (LIM) provides a promising way to probe cosmology, reionization and galaxy evolution. However, its sensitivity to cosmology and astrophysics at the same time is also a nuisance. Here we develop a comprehensive framework for modelling the LIM power spectrum, which includes redshift space distortions and the Alcock-Paczynski effect. We then identify and isolate degeneracies with astrophysics so that they can be marginalized over. We study the gains of using the multipole expansion of the anisotropic power spectrum, providing an accurate analytic expression for their covariance, and find a 10%-60% increase in the precision of the baryon acoustic oscillation scale measurements when including the hexadecapole in the analysis. We discuss different observational strategies when targeting other cosmological parameters, such as the sum of neutrino masses or primordial non-Gaussianity, finding that fewer and wider bins are typically more optimal. Overall, our formalism facilitates an optimal extraction of cosmological constraints robust to astrophysics.
21 pages; 6 figures. Matches published version
References in corpus (110)
- Efficient Computation of CMB anisotropies in closed FRW models
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- LOFAR: The LOw-Frequency ARray
- The CO-to-H2 Conversion Factor
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Early Dark Energy Can Resolve The Hubble Tension
- The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- The trouble with
- Hydrogen Epoch of Reionization Array (HERA)
- New physics in light of the tension: an alternative view
- Early dark energy, the Hubble-parameter tension, and the string axiverse
- Fundamental Physics with the Square Kilometre Array
- The effect of primordial non-Gaussianity on halo bias
- The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
- Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- Late-time cosmology with 21cm intensity mapping experiments
- The abundance of high-redshift objects as a probe of non-Gaussian initial conditions
- Acoustic Dark Energy: Potential Conversion of the Hubble Tension
- HI intensity mapping : a single dish approach
- Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
- Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the tension
- The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
- A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey
- Ingredients for 21cm intensity mapping
- Intensity Mapping with Carbon Monoxide Emission Lines and the Redshifted 21 cm Line
- Cosmology with the SPHEREX All-Sky Spectral Survey
- Late universe decaying dark matter can relieve the H_0 tension
- A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
- HIRAX: A Probe of Dark Energy and Radio Transients
- Twenty-one centimeter tomography with foregrounds
- Line-Intensity Mapping: 2017 Status Report
- The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range
- Rock 'n' Roll Solutions to the Hubble Tension
- Gaussian covariance matrices for anisotropic galaxy clustering measurements
- Primordial non-Gaussianity from the large scale structure
- A local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder
- Foregrounds for 21cm Observations of Neutral Gas at High Redshift
- Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly
- Modeling Biased Tracers at the Field Level
- Constraining Anisotropic Baryon Oscillations
- The promising future of a robust cosmological neutrino mass measurement
- Axion-Dilaton Destabilization and the Hubble Tension
- Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
- COPSS II: The Molecular Gas Content of Ten Million Cubic Megaparsecs at
- Intensity Mapping of Lyman-alpha Emission During the Epoch of Reionization
- 21-cm Fluctuations from Charged Dark Matter
- The HETDEX Pilot Survey V: The Physical Origin of Lyman-alpha Emitters Probed by Near-infrared Spectroscopy
- Intensity Mapping across Cosmic Times with the Lyman-Alpha Line
- Reconstructing Gravity on Cosmological Scales
- On Removing Interloper Contamination from Intensity Mapping Power Spectrum Measurements
- Cross-correlations as a cosmological carbon monoxide detector
- Bias due to neutrinos must not uncorrect'd go
- High-redshift post-reionization cosmology with 21cm intensity mapping
- Carbon Monoxide Intensity Mapping at Moderate Redshifts
- Spectral Line De-confusion in an Intensity Mapping Survey
- Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
- Constraining Primordial Non-Gaussianity with High-Redshift Probes
- MeerKLASS: MeerKAT Large Area Synoptic Survey
- HI and cosmological constraints from intensity mapping, optical, and CMB surveys
- Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
- Search for CII Emission on Cosmological Scales at Redshift Z~2.6
- Dissecting the high-z interstellar medium through intensity mapping cross-correlations
- A Standard Ruler at Cosmic Dawn
- Constraining the evolution of CII intensity through the end stages of reionization
- Constraining the CO intensity mapping power spectrum at intermediate redshifts
- Model independent inference of the expansion history and implications for the growth of structure
- Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
- Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
- Determining the HI content of galaxies via intensity mapping cross-correlations
- A Foreground Masking Strategy for [CII] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift
- Biases from neutrino bias: to worry or not to worry?
- Dark matter and halo bispectrum in redshift space: theory and applications
- Intensity mapping of H-alpha, H-beta, [OII] and [OIII] lines at z<5
- Insights from probability distribution functions of intensity maps
- Joint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAP
- First Results from COPSS: The CO Power Spectrum Survey
- Evidence for CII diffuse line emission at redshift
- Shot noise and biased tracers: a new look at the halo model
- Astrophysics and Cosmology with Line-Intensity Mapping
- Probing the Intergalactic Medium with Ly and 21 cm Fluctuations
- Lensing reconstruction from line intensity maps: the impact of gravitational nonlinearity
- Optimal Redshift Weighting For Baryon Acoustic Oscillations
- Weak Lensing of Intensity Mapping: the Cosmic Infrared Background
- Intensity mapping cross-correlations II: HI halo models including shot noise
- Observing AGN feedback with CO intensity mapping
- Optimising primordial non-Gaussianity measurements from galaxy surveys
- Measuring the growth of structure with intensity mapping surveys
- Synergies between intensity maps of hydrogen lines
- The high redshift star-formation history from carbon-monoxide intensity maps
- Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
- Constraining the Expansion History and Early Dark Energy with Line Intensity Mapping
- Extracting bias using the cross-bispectrum: An EoR and 21 cm-[CII]-[CII] case study
- Power spectrum modelling of galaxy and radio intensity maps including observational effects
- Anisotropic halo assembly bias and redshift-space distortions
- Probing Cosmic Origins with CO and [CII] Emission Lines
- Feeding cosmic star formation: Exploring high-redshift molecular gas with CO intensity mapping
- Canceling out intensity mapping foregrounds
- General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast
- Synergies between radio, optical and microwave observations at high redshift
- Probing CDM cosmology with the Evolutionary Map of the Universe survey
- A new estimator for gravitational lensing using galaxy and intensity mapping surveys
- Cosmic Dawn Intensity Mapper
- A partial inventory of observational anisotropies in single-dish line-intensity mapping
- Exploring the dusty star-formation in the early Universe using intensity mapping
- The Origins Space Telescope (OST) Mission Concept Study Interim Report
- A next-generation Very Large Array
Cited by in corpus (64)
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Line-Intensity Mapping: Theory Review
- The trouble beyond and the new cosmic triangles
- Robustness of baryon acoustic oscillation constraints for early-Universe modifications to CDM
- Intensity Mapping as a Probe of Axion Dark Matter
- The Cosmic Expansion History from Line-Intensity Mapping
- Strategies to Detect Dark-Matter Decays with Line-Intensity Mapping
- Beware of commonly used approximations II: estimating systematic biases in the best-fit parameters
- The cosmic optical background excess, dark matter, and line-intensity mapping
- Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly
- On cosmological signatures of baryons-dark energy elastic couplings
- COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization
- Detecting the relativistic bispectrum in 21cm intensity maps
- Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
- The Experiment for Cryogenic Large-aperture Intensity Mapping (EXCLAIM)
- Detecting the radiative decay of the cosmic neutrino background with line-intensity mapping
- Multipole expansion for HI intensity mapping experiments: simulations and modelling
- Intensity mapping from the sky: synergizing the joint potential of [OIII] and [CII] surveys at reionization
- COMAP Early Science: IV. Power Spectrum Methodology and Results
- Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
- A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
- Coupling parsec and gigaparsec scales: primordial non-Gaussianity with multi-tracer intensity mapping
- Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
- The HI intensity mapping bispectrum including observational effects
- Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
- Kinetic Sunyaev-Zel'dovich tomography with line-intensity mapping
- Constraining primordial non-Gaussianity by combining next-generation galaxy and 21 cm intensity mapping surveys
- Small-scale primordial fluctuations in the 21cm Dark Ages signal
- Beyond CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
- The local PNG bias of neutral Hydrogen,
- Cosmological Probes of Structure Growth and Tests of Gravity
- Measuring the cosmic expansion rate using 21-cm velocity acoustic oscillations
- On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
- Forecasts and Statistical Insights for Line Intensity Mapping Cross-Correlations: A Case Study with 21cm x [CII]
- A multi-tracer empirically-driven approach to line-intensity mapping lightcones
- Enlightening the dark ages with dark matter
- Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
- Extragalactic Science with the Experiment for Cryogenic Large-aperture Intensity Mapping
- Unveiling cosmological information on small scales with line intensity mapping
- Exploration of 3D wavelet scattering transform coefficients for line-intensity mapping measurements
- Intensity Mapping without Cosmic Variance
- Optical Design of the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)
- Antisymmetric cross-correlation of line-intensity maps as a probe of reionization
- Mapping the Universe in HD
- Unveiling the Universe with Emerging Cosmological Probes
- Towards Accurate Modeling of Line-Intensity Mapping One-Point Statistics: Including Extended Profiles
- Bayesian Multi-line Intensity Mapping
- On the contributions of extragalactic CO emission lines to ground-based CMB observations
- Probing the Epoch of Reionization using synergies of line intensity mapping
- Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
- Mixing Bispectrum Multipoles Under Geometric Distortions
- Constraining the Star Formation Rate using Joint CIB Continuum and [CII] Intensity Mapping
- Towards a multi-tracer neutrino mass measurement with line-intensity mapping
- Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
- Mapping Large-Scale-Structure Evolution over Cosmic Times
- Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
- Superfluid-tight cryogenic receiver with continuous sub-Kelvin cooling for EXCLAIM
- oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
- Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
- Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
- A Beginner's Guide to Line Intensity Mapping Power Spectra
- Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
- Probing the warm dark matter mass with [C II] intensity mapping
- Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys