The Statistical Significance of the "Dark Flow"
arXiv:0910.4233 · doi:10.1088/0004-637X/707/1/L42
Abstract
We revisit the statistical significance of the "dark flow" presented in Kashlinsky et al. (2009). We do not find a statistically significant detection of a bulk flow. Instead we find that CMB correlations between the 8 WMAP channels used in this analysis decrease the inferred significance of the detection to 0.7σ.
matches version in ApJL, Volume 707, Issue 1, pp. L42-L44 (2009)
References in corpus (2)
Cited by in corpus (33)
- Cosmological Parameters from Observations of Galaxy Clusters
- Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel'dovich Effect
- Is the Observable Universe Consistent with the Cosmological Principle?
- Dipoles in the Sky
- Measuring cosmic bulk flows with Type Ia Supernovae from the Nearby Supernova Factory
- The 6dF Galaxy Survey: Bulk Flows on Mpc scales
- Deriving accurate peculiar velocities (even at high redshift)
- The Local Hole revealed by galaxy counts and redshifts
- Hubble flow variance and the cosmic rest frame
- Measuring the dark flow with public X-ray cluster data
- Measuring the Galaxy Cluster Bulk Flow from WMAP data
- Measuring the cosmological bulk flow using the peculiar velocities of supernovae
- First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
- Probing the Dark Flow signal in WMAP 9 yr and PLANCK cosmic microwave background maps
- Probing bulk flow with nearby SNe Ia data
- Anisotropy of the galaxy cluster X-ray luminosity-temperature relation
- Galaxy Cluster Bulk Flows and Collision Velocities in QUMOND
- The dark flow induced small scale kinetic Sunyaev Zel'dovich effect
- One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
- Studying the Peculiar Velocity Bulk Flow in a Sparse Survey of Type-Ia SNe
- The error budget of the Dark Flow measurement
- Ultra-compact radio sources and the isotropy and homogeneity of the Universe
- On the Statistical Significance of the Bulk Flow Measured by the PLANCK Satellite
- Measuring Bulk Flow of Galaxy Clusters using Kinematic Sunyaev-Zel'dovich effect: Prediction for Planck
- Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
- Using measurements of the cosmic bulk flow to constrain Gravity
- The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
- Cluster mislocation in kinematic Sunyaev-Zel'dovich (kSZ) effect extraction
- Limits on Entanglement Effects in the String Landscape from Planck and BICEP/Keck Data
- Gravitational fluctuations of the galaxy distribution
- The Polarization Signature of Local Bulk Flows
- A large anisotropy in the sky distribution of 3CRR quasars and other radio galaxies
- Expected redshift drift for tilted observers