Optimal filters for the moving lens effect
arXiv:2006.03060 · doi:10.1103/PhysRevD.103.043536
Abstract
We assess the prospects for detecting the moving lens effect using cosmological surveys. The bulk motion of cosmological structure induces a small-scale dipolar temperature anisotropy of the cosmic microwave radiation (CMB), centered around halos and oriented along the transverse velocity field. We introduce a set of optimal filters for this signal, and forecast that a high significance detection can be made with upcoming experiments. We discuss the prospects for reconstructing the bulk transverse velocity field on large scales using matched filters, finding good agreement with previous work using quadratic estimators.
arXiv comment7 pages, 3 figures, v3: version published in PRD
References in corpus (24)
- The Structure of Cold Dark Matter Halos
- Halo Models of Large Scale Structure
- Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
- The Simons Observatory: Science goals and forecasts
- Weak Gravitational Lensing of the CMB
- The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
- New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z=0.2 to z=1
- A theoretical framework for combining techniques that probe the link between galaxies and dark matter
- Parameter constraints from cross-correlation of CMB lensing with galaxy clustering
- The Websky Extragalactic CMB Simulations
- Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
- Constraining local non-Gaussianities with kSZ tomography
- Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
- Kinetic Sunyaev-Zel'dovich effect from halo rotation
- Kinetic Sunyaev-Zeldovich effect from galaxy cluster rotation
- Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters
- Transverse Velocities with the Moving Lens Effect
- Towards testing CMB anomalies using the kinetic and polarized Sunyaev Zel'dovich effects
- Probing correlated compensated isocurvature perturbations using scale-dependent galaxy bias
- Pairwise Transverse Velocity Measurement with the Rees-Sciama Effect
- Forecasted constraints on modified gravity from Sunyaev Zel'dovich tomography
- Constraining the Rotational Kinematic Sunyaev-Zel'dovich Effect in Massive Galaxy Clusters
- Probing gaseous galactic halos through the rotational kSZ effect
- Primordial gravitational wave phenomenology with polarized Sunyaev Zel'dovich tomography
Cited by in corpus (16)
- The Benefits of CMB Delensing
- Cosmology with the moving lens effect
- Probing cosmic birefringence with polarized Sunyaev-Zel'dovich tomography
- The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
- Velocity reconstruction with the cosmic microwave background and galaxy surveys
- Primordial trispectrum from kSZ tomography
- Reconstructing Patchy Reionization with Deep Learning
- Understanding matched filters for precision cosmology
- Cosmology from the kinetic polarized Sunyaev Zel'dovich effect
- Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
- Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
- Unveiling Neutrino Halos with CMB Lensing
- Accurate relativistic observables from post-processing light cone catalogues
- Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
- Cosmological probes of helium reionization
- The Moving Lens Effect: Simulations, Forecasts and Foreground Mitigation