Reconstructing the projected gravitational potential of Abell 1689 from X-ray measurements
arXiv:1501.03080 · doi:10.1051/0004-6361/201323242
Abstract
Context. Galaxy clusters can be used as cosmological probes, but to this end, they need to be thoroughly understood. Combining all cluster observables in a consistent way will help us to understand their global properties and their internal structure. Aims. We provide proof of the concept that the projected gravitational potential of galaxy clusters can directly be reconstructed from X-ray observations. We also show that this joint analysis can be used to locally test the validity of the equilibrium assumptions in galaxy clusters. Methods. We used a newly developed reconstruction method, based on Richardson-Lucy deprojection, that allows reconstructing projected gravitational potentials of galaxy clusters directly from X-ray observations. We applied this algorithm to the well-studied cluster Abell 1689 and compared the gravitational potential reconstructed from X-ray observables to the potential obtained from gravitational lensing measurements. [...] Results. Assuming spherical symmetry and hydrostatic equilibrium, the potentials recovered from gravitational lensing and from X-ray emission agree very well beyond 500 kpc. Owing to the fact that the Richardson-Lucy deprojection algorithm allows deprojecting each line of sight independently, this result may indicate that non-gravitational effects and/or asphericity are strong in the central regions of the clusters. Conclusions. We demonstrate the robustness of the potential reconstruction method based on the Richardson-Lucy deprojection algorithm and show that gravitational lensing and X-ray emission lead to consistent gravitational potentials. Our results illustrate the power of combining galaxy-cluster observables in a single, non-parametric, joint reconstruction of consistent cluster potentials that can be used to locally constrain the physical state of the gas.
arXiv comment8 pages, 4 figures. Accepted in A&A
References in corpus (41)
- A Universal Density Profile from Hierarchical Clustering
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions
- Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
- X-ray Spectroscopy of Cooling Clusters
- The Evolution of X-ray Clusters and the Entropy of the Intra Cluster Medium
- Residual Gas Motions in the Intracluster Medium and Bias in Hydrostatic Measurements of Mass Profiles of Clusters
- A Catalog of Galaxy Clusters Observed by XMM-Newton
- The Efficiency of Globular Cluster Formation
- The Surprisingly Steep Mass Profile of Abell 1689, from a Lensing Analysis of Subaru Images
- Resolving the discrepancy between X-ray and gravitational lensing mass measurements for clusters of galaxies
- Joint Analysis of Cluster Observations: II. Chandra/XMM-Newton X-ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies
- Outer Regions of the Cluster Gaseous Atmospheres
- Mass profiles of Galaxy Clusters from X-ray analysis
- Gas Clumping in the Outskirts of Lambda-CDM Clusters
- The gas distribution in the outer regions of galaxy clusters
- Gravitational Lensing in Clusters of Galaxies: New Clues Regarding the Dynamics of Intracluster Gas
- Suzaku Observation of Abell 1689: Anisotropic Temperature and Entropy Distributions Associated with the Large-Scale Structure
- Outskirts of Galaxy Clusters
- Quantifying properties of ICM inhomogeneities
- Iron Gradients in Cooling Flow Galaxies and Groups
- Combining weak and strong cluster lensing: Applications to simulations and MS 2137
- Evolution of the Merger Induced Hydrostatic Mass Bias in Galaxy Clusters
- Properties of gas clumps and gas clumping factor in the intra cluster medium
- Complex Structure of Galaxy Cluster Abell 1689: Evidence for a Merger from X-ray data?
- The X-ray/SZ view of the virial region. I. Thermodynamic properties
- Modeling Intra-Cluster Gas in Triaxial Dark Halos : An Analytical Approach
- Mass, shape and thermal properties of A1689 by a multi-wavelength X-ray, lensing and Sunyaev-Zel'dovich analysis
- Joint deprojection of Sunyaev-Zeldovich and X-ray images of galaxy clusters
- Reconstructing Three-dimensional Structure of Underlying Triaxial Dark Halos From Xray and Sunyaev-Zel'dovich Effect Observations of Galaxy Clusters
- Spherically Averaging Ellipsoidal Galaxy Clusters in X-Ray and Sunyaev-Zel'dovich Studies: II. Biases
- The complex velocity distribution of galaxies in Abell 1689: implications for mass modelling
- Triaxiality and non-thermal gas pressure in Abell 1689
- Discrepant Mass Estimates in the Cluster of Galaxies Abell 1689
- Chandra observation of Abell 1689: New determination of mass distribution and comparison to lensing measurements
- The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
- X-ray observations of PKS 0745-191 at the virial radius: Are we there yet?
- Spherically Averaging Ellipsoidal Galaxy Clusters in X-Ray and Sunyaev-Zel'dovich Studies: I. Analytical Relations
- Three-dimensional reconstruction of the intra-cluster medium
- Joint reconstruction of galaxy clusters from gravitational lensing and thermal gas I. Outline of a non-parametric method
- Reconstructing the projected gravitational potential of galaxy clusters from galaxy kinematics
Cited by in corpus (8)
- Limit on graviton mass from galaxy cluster Abell 1689
- Comparison of weak lensing by NFW and Einasto halos and systematic errors
- Free-form modelling of galaxy clusters: a Bayesian and data-driven approach
- Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel'dovich measurements
- Characterizing galaxy clusters by their gravitational potential: systematics of cluster potential reconstruction
- Triaxiality in galaxy clusters: Mass versus Potential reconstructions
- CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
- A short review on joint weak and strong cluster lens-mass reconstruction