Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
arXiv:2406.12979 · doi:10.1103/PhysRevD.111.043539
Abstract
Line-intensity mapping (LIM) offers an approach to obtain three-dimensional maps of the large-scale structure by collecting the aggregate emission from all emitters along the line of sight. The procedure hinges on reconstructing the radial positions of sources by relating the observed frequency to the rest-frame frequency of a target emission line. However, this step is hindered by `interloper-line' emission from different cosmological volumes that redshifts into the same observed frequency. In this work, we propose a model-independent technique to remove the contamination of line interlopers using their statistical correlation with external tracers of the large-scale structure, and identify the weights that minimize the variance of the cleaned field. Furthermore, we derive expressions for the resulting power spectra after applying our cleaning procedure, and validate them against simulations. We find that the cleaning performance improves as the correlation between the line interlopers and the external tracer increases, resulting in a gain in the signal-to-noise ratio of up to a factor 6 (2) for the auto- (cross-)power spectrum in idealized scenarios. This approach has the advantage of being model-independent, and is highly complementary to other techniques, as it removes large-scale clustering modes instead of individually masking the brightest sources of contamination.
Matches published version. 11 pages (+1 page appendices + references), 4 figures
References in corpus (78)
- LOFAR: The LOw-Frequency ARray
- The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
- Toward a halo mass function for precision cosmology: the limits of universality
- UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
- The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
- Hydrogen Epoch of Reionization Array (HERA)
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
- Data Analysis for Precision 21 cm Cosmology
- Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
- Delensing CMB Polarization with External Datasets
- HIRAX: A Probe of Dark Energy and Radio Transients
- The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array
- Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly
- Probing Reionization with the 21 cm-Galaxy Cross Power Spectrum
- The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
- Delensing the CMB with the Cosmic Infrared Background
- 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
- COPSS II: The Molecular Gas Content of Ten Million Cubic Megaparsecs at
- CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
- Line-Intensity Mapping: Theory Review
- On Removing Interloper Contamination from Intensity Mapping Power Spectrum Measurements
- A User's Guide to Extracting Cosmological Information from Line-Intensity Maps
- A wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast
- Spectral Line De-confusion in an Intensity Mapping Survey
- An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm
- COMAP Early Science: I. Overview
- Foreground contamination in Ly-alpha intensity mapping during the epoch of reionization
- Generating Log-normal Mock Catalog of Galaxies in Redshift Space
- A Standard Ruler at Cosmic Dawn
- Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
- CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
- A Foreground Masking Strategy for [CII] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift
- Nulling Tomography with Weak Gravitational Lensing
- Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
- Demonstrating the Feasibility of Line Intensity Mapping Using Mock Data of Galaxy Clustering from Simulations
- Intensity mapping of H-alpha, H-beta, [OII] and [OIII] lines at z<5
- Multitracer CMB delensing maps from Planck and WISE data
- Probing Cosmic Reionization and Molecular Gas Growth with TIME
- The Cosmic Expansion History from Line-Intensity Mapping
- The Simons Observatory: Constraining inflationary gravitational waves with multi-tracer B-mode delensing
- Evidence for CII diffuse line emission at redshift
- Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys
- Strategies to Detect Dark-Matter Decays with Line-Intensity Mapping
- Phase-Space Spectral Line De-confusion in Intensity Mapping
- Neutrino Properties with Ground-Based Millimeter-Wavelength Line Intensity Mapping
- Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
- Surface Brightness Profile of Lyman- Halos out to 320 kpc in HETDEX
- The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
- Interloper bias in future large-scale structure surveys
- Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
- Intensity Mapping in the Presence of Foregrounds and Correlated Continuum Emission
- Measuring the EoR Power Spectrum Without Measuring the EoR Power Spectrum
- Detecting the radiative decay of the cosmic neutrino background with line-intensity mapping
- Correcting correlation functions for redshift-dependent interloper contamination
- Power spectrum modelling of galaxy and radio intensity maps including observational effects
- Impact of internal-delensing biases on searches for primordial B-modes of CMB polarisation
- A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
- Modeling HI at the field level
- Deep learning for intensity mapping observations: Component extraction
- Kinetic Sunyaev-Zel'dovich tomography with line-intensity mapping
- Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
- Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
- Delensing the CMB with the cosmic infrared background: the impact of foregrounds
- Deep Learning for Line Intensity Mapping Observations: Information Extraction from Noisy Maps
- Lyα Halos around [O III]-Selected Galaxies in HETDEX
- A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing
- A multi-tracer empirically-driven approach to line-intensity mapping lightcones
- Probing early structure and model-independent neutrino mass with high-redshift CMB lensing mass maps
- Optimally Mapping Large-Scale Structures with Luminous Sources
- CONCERTO: Extracting the power spectrum of the [C II ] emission line
- Deep learning reconstruction of three-dimensional galaxy distributions with intensity mapping observations
- Antisymmetric cross-correlation of line-intensity maps as a probe of reionization
- SIMPLE: Simple Intensity Map Producer for Line Emission
- Bayesian Multi-line Intensity Mapping
- Towards Accurate Modeling of Line-Intensity Mapping One-Point Statistics: Including Extended Profiles
- Model independent variance cancellation in CMB lensing cross-correlations