Sunyaev-Zeldovich signal processing and temperature-velocity moment method for individual clusters
arXiv:1211.3206 · doi:10.1093/mnras/stt110
Abstract
Future high resolution, high sensitivity Sunyaev-Zeldovich (SZ) observations of individual clusters will provide an exciting opportunity to answer specific questions about the dynamical state of the intra-cluster medium (ICM). In this paper we develop a new method that clearly shows the connection of the SZ signal with the underlying cluster model. We include relativistic temperature and kinematic corrections in the single-scattering approximation, allowing studies of hot clusters. In our approach, particular moments of the temperature and velocity field along the line-of-sight determine the precise spectral shape and morphology of the SZ signal. We illustrate how to apply our method to different cluster models, highlighting parameter degeneracies and instrumental effects that are important for interpreting future high-resolution SZ data. Our analysis shows that line-of-sight temperature variations can introduce significant biases in the derived SZ temperature and peculiar velocity. We furthermore discuss how the position of the SZ null is affected by the cluster's temperature and velocity structure. Our computations indicate that the SZ signal around the null alone is rather insensitive to different cluster models and that high frequency channels add a large leverage in this respect. We also apply our method to recent high sensitivity SZ data of the Bullet cluster, showing how the results can be linked to line-of-sight variations in the electron temperature. The tools developed here as part of SZpack should be useful for analyzing high-resolution SZ data and computing SZ maps from simulated clusters.
16 pages, 12 figures, 2 tables, accepted version (MNRAS)
References in corpus (9)
- Shocks and cold fronts in galaxy clusters
- Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
- Effects of Baryons and Dissipation on the Matter Power Spectrum
- A fast and accurate method for computing the Sunyaev-Zeldovich signal of hot galaxy clusters
- A Multi-wavelength Study of the Sunyaev-Zel'dovich Effect in the Triple-Merger Cluster MACS J0717.5+3745 with MUSTANG and Bolocam
- Non-Equilibrium Electrons and the Sunyaev-Zel'dovich Effect of Galaxy Clusters
- The first measurement of temperature standard deviation along the line-of-sight in galaxy clusters
- Theory of Compton scattering by anisotropic electrons
- Study on the Solutions of the Sunyaev-Zeldovich Effect for Clusters of Galaxies
Cited by in corpus (49)
- Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects: A Millimetre/Submillimetre Probe of the Warm and Hot Universe
- Weighing the Giants V: Galaxy Cluster Scaling Relations
- Rethinking CMB foregrounds: systematic extension of foreground parameterizations
- Which spectral distortions does CDM actually predict?
- Distinguishing different scenarios of early energy release with spectral distortions of the cosmic microwave background
- Taking the Universe's Temperature with Spectral Distortions of the Cosmic Microwave Background
- The synergy between CMB spectral distortions and anisotropies
- Prospects for Measuring Cosmic Microwave Background Spectral Distortions in the Presence of Foregrounds
- Peeling off foregrounds with the constrained moment ILC method to unveil primordial CMB -modes
- Planck's view on the spectrum of the Sunyaev-Zeldovich effect
- Cosmological constraints on decaying axion-like particles: a global analysis
- Can we neglect relativistic temperature corrections in the Planck thermal SZ analysis?
- Tests of the CMB temperature-redshift relation, CMB spectral distortions and why adiabatic photon production is hard
- Imaging the Thermal and Kinematic Sunyaev-Zel'dovich Effect Signals in a Sample of Ten Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities
- Relativistic SZ temperature scaling relations of groups and clusters derived from the BAHAMAS and MACSIS simulations
- Mapping the relativistic electron gas temperature across the sky
- Combining ILC and moment expansion techniques for extracting average-sky signals and CMB anisotropies
- High precision modeling of polarized signals: Moment expansion method generalized to spin-2 fields
- A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
- Peculiar Velocity Constraints from Five-Band SZ Effect Measurements Towards RX J1347.5-1145 with MUSIC and Bolocam from the CSO
- Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton -map analysis
- Measuring using X-ray and SZ effect observations of dynamically relaxed galaxy clusters
- Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
- Unlocking the synergy between CMB spectral distortions and anisotropies
- Multiple scattering Sunyaev-Zeldovich signal I: lowest order effect
- Multiple scattering Sunyaev-Zeldovich signal II: relativistic effects
- Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
- Percent-level constraints on baryonic feedback with spectral distortion measurements
- Refined modelling of the radio SZ signal: kinematic terms, relativistic temperature corrections and anisotropies in the radio background
- The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 0.60 and M M
- Cosmology from the kinetic polarized Sunyaev Zel'dovich effect
- Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
- Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
- Measurement of the Relativistic Sunyaev-Zeldovich Corrections in RX J1347.5-1145
- Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
- Stokes parameters spectral distortions due to the Sunyaev-Zel'dovich effect and an independent estimation of the CMB low multipoles
- How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
- Polarization of the Sunyaev-Zel'dovich effect: relativistic imprint of thermal and non-thermal plasma
- A 15.5 GHz detection of the galaxy cluster minihalo in RXJ1720.1+2638
- Bayesian recalibration of Planck galaxy cluster scaling relations including relativistic Sunyaev-Zel'dovich corrections
- Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
- Effects of boosting on extragalactic components: methods and statistical studies
- SPECTER: An Instrument Concept for CMB Spectral Distortion Measurements with Enhanced Sensitivity
- The FLAMINGO simulations data release
- Temperature measurements with the relativistic Sunyaev-Zel'dovich effect
- Fully Relativistic Derivation of the Thermal Sunyaev-Zel'dovich Effect
- Relativistic SZ maps and electron gas temperature spectroscopy
- The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745
- Galaxy cluster temperature maps from joint X-ray and SZ maps with The Three Hundred hydrodynamical simulations