Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos
arXiv:1411.7999 · doi:10.1103/PhysRevLett.114.151302
Abstract
We present evidence of the gravitational lensing of the cosmic microwave background by solar mass dark matter halos. Lensing convergence maps from the Atacama Cosmology Telescope Polarimeter (ACTPol) are stacked at the positions of around 12,000 optically-selected CMASS galaxies from the SDSS-III/BOSS survey. The mean lensing signal is consistent with simulated dark matter halo profiles, and is favored over a null signal at 3.2 sigma significance. This result demonstrates the potential of microwave background lensing to probe the dark matter distribution in galaxy group and galaxy cluster halos.
9 pages, 3 figures, accepted by PRL, author list corrected
References in corpus (10)
- The 2.5 m Telescope of the Sloan Digital Sky Survey
- Detection of Gravitational Lensing in the Cosmic Microwave Background
- Correlation of CMB with large-scale structure: II. Weak lensing
- ACTPol: A polarization-sensitive receiver for the Atacama Cosmology Telescope
- Precision Epoch of Reionization studies with next-generation CMB experiments
- A Measurement of the Correlation of Galaxy Surveys with CMB Lensing Convergence Maps from the South Pole Telescope
- Weighing obscured and unobscured quasar hosts with the CMB
- The Atacama Cosmology Telescope: Cross Correlation with Planck maps
- Improved estimation of cluster mass profiles from the cosmic microwave background
- CMB Cluster Lensing: Cosmography with the Longest Lever Arm
Cited by in corpus (31)
- CMB-S4 Science Case, Reference Design, and Project Plan
- The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
- The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies
- Fundamental Physics from Future Weak-Lensing Calibrated Sunyaev-Zel'dovich Galaxy Cluster Counts
- CMB Lensing Beyond the Power Spectrum: Cosmological Constraints from the One-Point PDF and Peak Counts
- Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
- Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
- POLOCALC: a Novel Method to Measure the Absolute Polarization Orientation of the Cosmic Microwave Background
- The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
- Calibrating Cluster Number Counts with CMB lensing
- DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing
- Constraining Dark Matter properties with the first generation of stars
- The Atacama Cosmology Telescope: Weighing distant clusters with the most ancient light
- Multicomponent multiscatter capture of Dark Matter
- Mass Estimation of Galaxy Clusters with Deep Learning II: CMB Cluster Lensing
- Dark Energy Survey Year 3 results: imprints of cosmic voids and superclusters in the Planck CMB lensing map
- Cross-correlation of Planck CMB lensing with DESI galaxy groups
- Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
- Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
- Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
- Probing the origin of our Universe through cosmic microwave background constraints on gravitational waves
- Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations
- The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
- The CMB lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog
- A measurement of cluster masses using Planck and SPT-SZ CMB lensing
- A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
- The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
- Prospects for studying the mass and gas in protoclusters with future CMB observations
- The mass and galaxy distribution around SZ-selected clusters
- Supermassive Dark Stars and their remnants as a possible solution to three recent cosmic dawn puzzles
- Graphene-Insulator-Superconductor junctions as thermoelectric bolometers